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@ARTICLE{Koester:1998,
author = {{Koester}, D. and {Dreizler}, S. and {Weidemann}, V. and {Allard}, N.~F.
},
title = "{Search for rotation in white dwarfs}",
journal = {\aap},
keywords = {STARS: WHITE DWARFS, STARS: ROTATION, STARS: MAGNETIC FIELDS},
year = 1998,
month = oct,
volume = 338,
pages = {612-622},
adsurl = {http://adsabs.harvard.edu/abs/1998A%26A...338..612K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Lecoanet:2013,
author = {{Lecoanet}, D. and {Quataert}, E.},
title = "{Internal gravity wave excitation by turbulent convection}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1210.4547},
primaryClass = "astro-ph.SR",
keywords = {convection, hydrodynamics, waves, Sun: oscillations},
year = 2013,
month = apr,
volume = 430,
pages = {2363-2376},
doi = {10.1093/mnras/stt055},
adsurl = {http://adsabs.harvard.edu/abs/2013MNRAS.430.2363L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Rogers:2013,
author = {{Rogers}, T.~M. and {Lin}, D.~N.~C. and {McElwaine}, J.~N. and
{Lau}, H.~H.~B.},
title = "{Internal Gravity Waves in Massive Stars: Angular Momentum Transport}",
journal = {\apj},
archivePrefix = "arXiv",
eprint = {1306.3262},
primaryClass = "astro-ph.SR",
keywords = {hydrodynamics, stars: interiors, stars: rotation, waves },
year = 2013,
month = jul,
volume = 772,
eid = {21},
pages = {21},
doi = {10.1088/0004-637X/772/1/21},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...772...21R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@INPROCEEDINGS{Grosjean:2013,
author = {{Grosjean}, M. and {Dupret}, M. and {Belkacem}, K. and {Montalban}, J. and {Samadi}, R.},
title = {{Energetical aspects of solar-like oscillations in red giants}},
booktitle = {Precision Asteroseismology},
year = {2013},
series = {Proceedings IAU Symposium},
volume = {301},
}
@ARTICLE{Nielsen:2013,
author = {{Nielsen}, M.~B. and {Gizon}, L. and {Schunker}, H. and {Karoff}, C.
},
title = "{Rotation periods of 12 000 main-sequence Kepler stars: Dependence on stellar spectral type and comparison with v sin i observations}",
journal = {\aap},
archivePrefix = "arXiv",
eprint = {1305.5721},
primaryClass = "astro-ph.SR",
keywords = {stars: rotation, starspots, stars: late-type},
year = 2013,
month = sep,
volume = 557,
eid = {L10},
pages = {L10},
doi = {10.1051/0004-6361/201321912},
adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...557L..10N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Baran:2012,
author = {{Baran}, A.~S. and {Reed}, M.~D. and {Stello}, D. and {{\O}stensen}, R.~H. and
{Telting}, J.~H. and {Pak{\v s}tien{\"e}}, E. and {O'Toole}, S.~J. and
{Silvotti}, R. and {Degroote}, P. and {Bloemen}, S. and {Hu}, H. and
{Van Grootel}, V. and {Clarke}, B.~D. and {Van Cleve}, J. and
{Thompson}, S.~E. and {Kawaler}, S.~D.},
title = "{A pulsation zoo in the hot subdwarf B star KIC 10139564 observed by Kepler}",
journal = {\mnras},
archivePrefix = "arXiv",
eprint = {1206.3841},
primaryClass = "astro-ph.SR",
keywords = {asteroseismology, techniques: photometric, stars: oscillation, subdwarfs },
year = 2012,
month = aug,
volume = 424,
pages = {2686-2700},
doi = {10.1111/j.1365-2966.2012.21355.x},
adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.424.2686B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Kawaler:2005,
author = {{Kawaler}, S.~D. and {Hostler}, S.~R.},
title = "{Internal Rotation of Subdwarf B Stars: Limiting Cases and Asteroseismological Consequences}",
journal = {\apj},
eprint = {astro-ph/0411314},
keywords = {Stars: Horizontal-Branch, Stars: Oscillations, Stars: Rotation, Stars: Variables: Other, Stars: Subdwarfs},
year = 2005,
month = mar,
volume = 621,
pages = {432-444},
doi = {10.1086/427403},
adsurl = {http://adsabs.harvard.edu/abs/2005ApJ...621..432K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Tayar:2013,
author = {{Tayar}, J. and {Pinsonneault}, M.~H.},
title = "{Implications of Rapid Core Rotation in Red Giants for Internal Angular Momentum Transport in Stars}",
journal = {\apjl},
archivePrefix = "arXiv",
eprint = {1306.3986},
primaryClass = "astro-ph.SR",
keywords = {stars: evolution, stars: rotation },
year = 2013,
month = sep,
volume = 775,
eid = {L1},
pages = {L1},
doi = {10.1088/2041-8205/775/1/L1},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...775L...1T},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Zahn:1997,
author = {{Zahn}, J.-P. and {Talon}, S. and {Matias}, J.},
title = {{Angular momentum transport by internal waves in the solar interior.}},
journal = {\aap},
eprint = {astro-ph/9611189},
keywords = {HYDRODYNAMICS, TURBULENCE, SUN: INTERIOR: ROTATION, STARS: INTERIORS: ROTATION},
year = {1997},
month = {jun},
volume = {322},
pages = {320-328},
adsurl = {http://adsabs.harvard.edu/abs/1997A%26A...322..320Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Charbonnel:2005,
author = {{Charbonnel}, C. and {Talon}, S.},
title = {{Influence of Gravity Waves on the Internal Rotation and Li Abundance of Solar-Type Stars}},
journal = {Science},
eprint = {arXiv:astro-ph/0511265},
year = {2005},
month = {sep},
volume = {309},
pages = {2189-2191},
doi = {10.1126/science.1116849},
adsurl = {http://adsabs.harvard.edu/abs/2005Sci...309.2189C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Bloecker:1995,
author = {{Bloecker}, T.},
title = {{Stellar evolution of low and intermediate-mass stars. I. Mass loss on the AGB and its consequences for stellar evolution.}},
journal = {\aap},
keywords = {STARS: EVOLUTION, STARS: MASS LOSS, STARS: AGB, POST-AGB},
year = {1995},
month = {may},
volume = {297},
pages = {727},
adsurl = {http://adsabs.harvard.edu/abs/1995A%26A...297..727B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Denissenkov:2011,
author = {{Denissenkov}, P.~A. and {Merryfield}, W.~J.},
title = {{Thermohaline Mixing: Does it Really Govern the Atmospheric Chemical Composition of Low-mass Red Giants?}},
journal = {\apjl},
archiveprefix = {arXiv},
eprint = {1011.2191},
primaryclass = {astro-ph.SR},
keywords = {stars: abundances, stars: evolution, stars: interiors},
year = {2011},
month = {jan},
volume = {727},
eid = {L8},
pages = {L8},
doi = {10.1088/2041-8205/727/1/L8},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...727L...8D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Brown:2013,
author = {{Brown}, J.~M. and {Garaud}, P. and {Stellmach}, S.},
title = {{Chemical Transport and Spontaneous Layer Formation in Fingering Convection in Astrophysics}},
journal = {\apj},
archiveprefix = {arXiv},
eprint = {1212.1688},
primaryclass = {astro-ph.SR},
keywords = {convection, diffusion, hydrodynamics, instabilities, planet-star interactions, stars: evolution},
year = {2013},
month = {may},
volume = {768},
eid = {34},
pages = {34},
doi = {10.1088/0004-637X/768/1/34},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...768...34B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Traxler:2011,
author = {{Traxler}, A. and {Garaud}, P. and {Stellmach}, S.},
title = {{Numerically Determined Transport Laws for Fingering (''Thermohaline'') Convection in Astrophysics}},
journal = {\apjl},
archiveprefix = {arXiv},
eprint = {1011.3461},
primaryclass = {astro-ph.SR},
keywords = {hydrodynamics, instabilities, turbulence},
year = {2011},
month = {feb},
volume = {728},
eid = {L29},
pages = {L29},
doi = {10.1088/2041-8205/728/2/L29},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...728L..29T},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Cantiello:2010,
author = {{Cantiello}, M. and {Langer}, N.},
title = {{Thermohaline mixing in evolved low-mass stars}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {1006.1354},
primaryclass = {astro-ph.SR},
keywords = {stars: abundances, stars: evolution, stars: magnetic field, nuclear reactions, nucleosynthesis, abundances, stars: AGB and post-AGB, stars: rotation},
year = {2010},
month = {oct},
volume = {521},
eid = {A9},
pages = {A9},
doi = {10.1051/0004-6361/201014305},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...521A...9C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Charbonnel:2007,
author = {{Charbonnel}, C. and {Zahn}, J.-P.},
title = {{Thermohaline mixing: a physical mechanism governing the photospheric composition of low-mass giants}},
journal = {\aap},
eprint = {astro-ph/0703302},
keywords = {instabilities, stars: abundances, stars: interiors, hydrodynamics},
year = {2007},
month = {may},
volume = {467},
pages = {L15-L18},
doi = {10.1051/0004-6361:20077274},
adsurl = {http://adsabs.harvard.edu/abs/2007A%26A...467L..15C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Palacios:2006,
author = {{Palacios}, A. and {Charbonnel}, C. and {Talon}, S. and {Siess}, L.},
title = {{Rotational mixing in low-mass stars. II. Self-consistent models of Pop II RGB stars}},
journal = {\aap},
eprint = {astro-ph/0602389},
keywords = {stars: evolution, stars: interiors, stars: rotation, stars: abundances, hydrodynamics, turbulence},
year = {2006},
month = {jul},
volume = {453},
pages = {261-278},
doi = {10.1051/0004-6361:20053065},
adsurl = {http://adsabs.harvard.edu/abs/2006A%26A...453..261P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Nordhaus:2008,
author = {{Nordhaus}, J. and {Busso}, M. and {Wasserburg}, G.~J. and {Blackman}, E.~G. and {Palmerini}, S.},
title = {{Magnetic Mixing in Red Giant and Asymptotic Giant Branch Stars}},
journal = {\apjl},
archiveprefix = {arXiv},
eprint = {0806.3933},
keywords = {Magnetohydrodynamics: MHD, Stars: Abundances, Stars: AGB and Post-AGB, Stars: Interiors, Stars: Magnetic Fields, Stars: Rotation},
year = {2008},
month = {sep},
volume = {684},
pages = {L29-L32},
doi = {10.1086/591963},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...684L..29N},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@BOOK{Aerts:2010,
author = {{Aerts}, C. and {Christensen-Dalsgaard}, J. and {Kurtz}, D.~W.},
title = {{Asteroseismology}},
keywords = {Physics, Astronomy, Astrophysics and Cosmology},
booktitle = {Asteroseismology, Astronomy and Astrophysics Library.~ISBN 978-1-4020-5178-4.~Springer Science+Business Media B.V., 2010, p.},
year = {2010},
adsurl = {http://adsabs.harvard.edu/abs/2010aste.book.....A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Gratton:2000,
author = {{Gratton}, R.~G. and {Sneden}, C. and {Carretta}, E. and {Bragaglia}, A.},
title = {{Mixing along the red giant branch in metal-poor field stars}},
journal = {\aap},
keywords = {STARS: HERTZSPRUNG-RUSSEL (HR) AND C-M DIAGRAMS, STARS: EVOLUTION, STARS: POPULATION II, GALAXY: GLOBULAR CLUSTERS: GENERAL},
year = {2000},
month = {feb},
volume = {354},
pages = {169-187},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...354..169G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Spada:2010,
author = {{Spada}, F. and {Lanzafame}, A.~C. and {Lanza}, A.~F.},
title = {{A semi-analytic approach to angular momentum transport in stellar radiative interiors}},
journal = {\mnras},
keywords = {MHD, methods: analytical, methods: numerical, stars: late-type, stars: magnetic fields, stars: rotation},
year = {2010},
month = {may},
volume = {404},
pages = {641-660},
doi = {10.1111/j.1365-2966.2010.16325.x},
adsurl = {http://adsabs.harvard.edu/abs/2010MNRAS.404..641S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Gough:1998,
author = {{Gough}, D.~O. and {McIntyre}, M.~E.},
title = {{Inevitability of a magnetic field in the Sun's radiative interior}},
journal = {\nat},
year = {1998},
month = {aug},
volume = {394},
pages = {755-757},
doi = {10.1038/29472},
adsurl = {http://adsabs.harvard.edu/abs/1998Natur.394..755G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Dupret:2009,
author = {{Dupret}, M.-A. and {Belkacem}, K. and {Samadi}, R. and {Montalban}, J. and {Moreira}, O. and {Miglio}, A. and {Godart}, M. and {Ventura}, P. and {Ludwig}, H.-G. and {Grigahc{\`e}ne}, A. and {Goupil}, M.-J. and {Noels}, A. and {Caffau}, E.},
title = {{Theoretical amplitudes and lifetimes of non-radial solar-like oscillations in red giants}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {0906.3951},
primaryclass = {astro-ph.SR},
keywords = {stars: oscillations, stars: interiors, convection},
year = {2009},
month = {oct},
volume = {506},
pages = {57-67},
doi = {10.1051/0004-6361/200911713},
adsurl = {http://adsabs.harvard.edu/abs/2009A%26A...506...57D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{JCD:2008,
author = {{Christensen-Dalsgaard}, J.},
title = {{ADIPLS{\mdash}the Aarhus adiabatic oscillation package}},
journal = {\apss},
archiveprefix = {arXiv},
eprint = {0710.3106},
keywords = {Stars: oscillations, Numerical methods, Asteroseismology},
year = {2008},
month = {aug},
volume = {316},
pages = {113-120},
doi = {10.1007/s10509-007-9689-z},
adsurl = {http://adsabs.harvard.edu/abs/2008Ap%26SS.316..113C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Ceillier:2013,
author = {{Ceillier}, T. and {Eggenberger}, P. and {Garc{\'{\i}}a}, R.~A. and {Mathis}, S.},
title = {{Understanding angular momentum transport in red giants: the case of KIC 7341231}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {1305.5630},
primaryclass = {astro-ph.SR},
keywords = {stars: rotation, stars: oscillations, stars: evolution},
year = {2013},
month = {jul},
volume = {555},
eid = {A54},
pages = {A54},
doi = {10.1051/0004-6361/201321473},
adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...555A..54C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@BOOK{KW:1990,
author = {{Kippenhahn}, R. and {Weigert}, A.},
title = {{Stellar Structure and Evolution}},
keywords = {STELLAR STRUCTURE, STELLAR EVOLUTION},
booktitle = {Stellar Structure and Evolution, XVI, 468 pp.~192 figs..~ Springer-Verlag Berlin Heidelberg New York.~Also Astronomy and Astrophysics Library},
year = {1990},
adsurl = {http://adsabs.harvard.edu/abs/1990sse..book.....K},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Deheuvels:2012,
author = {{Deheuvels}, S. and {Garc{\'{\i}}a}, R.~A. and {Chaplin}, W.~J. and {Basu}, S. and {Antia}, H.~M. and {Appourchaux}, T. and {Benomar}, O. and {Davies}, G.~R. and {Elsworth}, Y. and {Gizon}, L. and {Goupil}, M.~J. and {Reese}, D.~R. and {Regulo}, C. and {Schou}, J. and {Stahn}, T. and {Casagrande}, L. and {Christensen-Dalsgaard}, J. and {Fischer}, D. and {Hekker}, S. and {Kjeldsen}, H. and {Mathur}, S. and {Mosser}, B. and {Pinsonneault}, M. and {Valenti}, J. and {Christiansen}, J.~L. and {Kinemuchi}, K. and {Mullally}, F.},
title = {{Seismic Evidence for a Rapidly Rotating Core in a Lower-giant-branch Star Observed with Kepler}},
journal = {\apj},
archiveprefix = {arXiv},
eprint = {1206.3312},
primaryclass = {astro-ph.SR},
keywords = {stars: evolution, stars: individual: KIC 7341231, stars: interiors, stars: oscillations},
year = {2012},
month = {sep},
volume = {756},
eid = {19},
pages = {19},
doi = {10.1088/0004-637X/756/1/19},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...756...19D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Mosser:2012,
author = {{Mosser}, B. and {Goupil}, M.~J. and {Belkacem}, K. and {Marques}, J.~P. and {Beck}, P.~G. and {Bloemen}, S. and {De Ridder}, J. and {Barban}, C. and {Deheuvels}, S. and {Elsworth}, Y. and {Hekker}, S. and {Kallinger}, T. and {Ouazzani}, R.~M. and {Pinsonneault}, M. and {Samadi}, R. and {Stello}, D. and {Garc{\'{\i}}a}, R.~A. and {Klaus}, T.~C. and {Li}, J. and {Mathur}, S. and {Morris}, R.~L.},
title = {{Spin down of the core rotation in red giants}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {1209.3336},
primaryclass = {astro-ph.SR},
keywords = {stars: oscillations, stars: interiors, stars: rotation, stars: late-type},
year = {2012},
month = {dec},
volume = {548},
eid = {A10},
pages = {A10},
doi = {10.1051/0004-6361/201220106},
adsurl = {http://adsabs.harvard.edu/abs/2012A%26A...548A..10M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Beck:2011,
author = {{Beck}, P.~G. and {Bedding}, T.~R. and {Mosser}, B. and {Stello}, D. and {Garcia}, R.~A. and {Kallinger}, T. and {Hekker}, S. and {Elsworth}, Y. and {Frandsen}, S. and {Carrier}, F. and {De Ridder}, J. and {Aerts}, C. and {White}, T.~R. and {Huber}, D. and {Dupret}, M.-A. and {Montalb{\'a}n}, J. and {Miglio}, A. and {Noels}, A. and {Chaplin}, W.~J. and {Kjeldsen}, H. and {Christensen-Dalsgaard}, J. and {Gilliland}, R.~L. and {Brown}, T.~M. and {Kawaler}, S.~D. and {Mathur}, S. and {Jenkins}, J.~M.},
title = {{Kepler Detected Gravity-Mode Period Spacings in a Red Giant Star}},
journal = {Science},
year = {2011},
month = {apr},
volume = {332},
pages = {205-},
doi = {10.1126/science.1201939},
adsurl = {http://adsabs.harvard.edu/abs/2011Sci...332..205B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Eggenberger:2005,
author = {{Eggenberger}, P. and {Maeder}, A. and {Meynet}, G.},
title = {{Stellar evolution with rotation and magnetic fields. IV. The solar rotation profile}},
journal = {\aap},
eprint = {astro-ph/0508455},
keywords = {stars: rotation, stars: magnetic fields, stars: evolution},
year = {2005},
month = {sep},
volume = {440},
pages = {L9-L12},
doi = {10.1051/0004-6361:200500156},
adsurl = {http://adsabs.harvard.edu/abs/2005A%26A...440L...9E},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Beck:2012,
author = {{Beck}, P.~G. and {Montalban}, J. and {Kallinger}, T. and {De Ridder}, J. and {Aerts}, C. and {Garc{\'{\i}}a}, R.~A. and {Hekker}, S. and {Dupret}, M.-A. and {Mosser}, B. and {Eggenberger}, P. and {Stello}, D. and {Elsworth}, Y. and {Frandsen}, S. and {Carrier}, F. and {Hillen}, M. and {Gruberbauer}, M. and {Christensen-Dalsgaard}, J. and {Miglio}, A. and {Valentini}, M. and {Bedding}, T.~R. and {Kjeldsen}, H. and {Girouard}, F.~R. and {Hall}, J.~R. and {Ibrahim}, K.~A.},
title = {{Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes}},
journal = {\nat},
archiveprefix = {arXiv},
eprint = {1112.2825},
primaryclass = {astro-ph.SR},
year = {2012},
month = {jan},
volume = {481},
pages = {55-57},
doi = {10.1038/nature10612},
adsurl = {http://adsabs.harvard.edu/abs/2012Natur.481...55B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Marques:2013,
author = {{Marques}, J.~P. and {Goupil}, M.~J. and {Lebreton}, Y. and {Talon}, S. and {Palacios}, A. and {Belkacem}, K. and {Ouazzani}, R.-M. and {Mosser}, B. and {Moya}, A. and {Morel}, P. and {Pichon}, B. and {Mathis}, S. and {Zahn}, J.-P. and {Turck-Chi{\`e}ze}, S. and {Nghiem}, P.~A.~P.},
title = {{Seismic diagnostics for transport of angular momentum in stars. I. Rotational splittings from the pre-main sequence to the red-giant branch}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {1211.1271},
primaryclass = {astro-ph.SR},
keywords = {stars: evolution, stars: interiors, stars: rotation, stars: oscillations},
year = {2013},
month = {jan},
volume = {549},
eid = {A74},
pages = {A74},
doi = {10.1051/0004-6361/201220211},
adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...549A..74M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Eggenberger:2012,
author = {{Eggenberger}, P. and {Montalb{\'a}n}, J. and {Miglio}, A.},
title = {{Angular momentum transport in stellar interiors constrained by rotational splittings of mixed modes in red giants}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {1207.1023},
primaryclass = {astro-ph.SR},
keywords = {stars: rotation, stars: oscillations},
year = {2012},
month = {aug},
volume = {544},
eid = {L4},
pages = {L4},
doi = {10.1051/0004-6361/201219729},
adsurl = {http://adsabs.harvard.edu/abs/2012A%26A...544L...4E},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Iglesias:1996,
author = {{Iglesias}, C.~A. and {Rogers}, F.~J.},
title = {{Updated Opal Opacities}},
journal = {\apj},
keywords = {ATOMIC DATA, ATOMIC PROCESSES, STARS: INTERIORS},
year = {1996},
month = {jun},
volume = {464},
pages = {943},
doi = {10.1086/177381},
adsurl = {http://adsabs.harvard.edu/abs/1996ApJ...464..943I},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Iglesias:1993,
author = {{Iglesias}, C.~A. and {Rogers}, F.~J.},
title = {{Radiative opacities for carbon- and oxygen-rich mixtures}},
journal = {\apj},
keywords = {CARBON ISOTOPES, HYDROGEN ISOTOPES, MAIN SEQUENCE STARS, OXYGEN ISOTOPES, STELLAR ENVELOPES, STELLAR EVOLUTION, ASYMPTOTIC GIANT BRANCH STARS, RADIATIVE TRANSFER, STELLAR STRUCTURE},
year = {1993},
month = {aug},
volume = {412},
pages = {752-760},
doi = {10.1086/172958},
adsurl = {http://adsabs.harvard.edu/abs/1993ApJ...412..752I},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Langer:1985,
author = {{Langer}, N. and {El Eid}, M.~F. and {Fricke}, K.~J.},
title = {{Evolution of massive stars with semiconvective diffusion}},
journal = {\aap},
keywords = {CONVECTIVE FLOW, STELLAR EVOLUTION, STELLAR MASS, STELLAR MODELS, SUPERMASSIVE STARS, TURBULENT DIFFUSION, HERTZSPRUNG-RUSSELL DIAGRAM, STELLAR COMPOSITION, STELLAR CORES, STELLAR STRUCTURE, STELLAR TEMPERATURE, TIME DEPENDENCE},
year = {1985},
month = {apr},
volume = {145},
pages = {179-191},
adsurl = {http://adsabs.harvard.edu/abs/1985A%26A...145..179L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Langer:1983,
author = {{Langer}, N. and {Fricke}, K.~J. and {Sugimoto}, D.},
title = {{Semiconvective diffusion and energy transport}},
journal = {\aap},
keywords = {ASTROPHYSICS, CONVECTION, DIFFUSION, ENERGY TRANSFER, STELLAR STRUCTURE, DIFFUSION COEFFICIENT, STELLAR INTERIORS, TEMPERATURE GRADIENTS},
year = {1983},
month = {sep},
volume = {126},
pages = {207},
adsurl = {http://adsabs.harvard.edu/abs/1983A%26A...126..207L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Henyey:1965,
author = {{Henyey}, L. and {Vardya}, M.~S. and {Bodenheimer}, P.},
title = {{Studies in Stellar Evolution. III. The Calculation of Model Envelopes.}},
journal = {\apj},
year = {1965},
month = {oct},
volume = {142},
pages = {841},
doi = {10.1086/148357},
adsurl = {http://adsabs.harvard.edu/abs/1965ApJ...142..841H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@INPROCEEDINGS{Asplund:2005,
author = {{Asplund}, M. and {Grevesse}, N. and {Sauval}, A.~J.},
title = {{The Solar Chemical Composition}},
booktitle = {Cosmic Abundances as Records of Stellar Evolution and Nucleosynthesis},
year = {2005},
series = {Astronomical Society of the Pacific Conference Series},
volume = {336},
editor = {{Barnes}, III, T.~G. and {Bash}, F.~N.},
month = {sep},
pages = {25},
adsurl = {http://adsabs.harvard.edu/abs/2005ASPC..336...25A},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Endal:1976,
author = {{Endal}, A.~S. and {Sofia}, S.},
title = {{The evolution of rotating stars. I - Method and exploratory calculations for a 7-solar-mass star}},
journal = {\apj},
keywords = {ANGULAR MOMENTUM, MAIN SEQUENCE STARS, MOMENTUM TRANSFER, STELLAR EVOLUTION, STELLAR MODELS, STELLAR ROTATION, ANGULAR DISTRIBUTION, APPROXIMATION, HERTZSPRUNG-RUSSELL DIAGRAM, MASS DISTRIBUTION, STELLAR MASS, STELLAR STRUCTURE, VELOCITY DISTRIBUTION},
year = {1976},
month = {nov},
volume = {210},
pages = {184-198},
doi = {10.1086/154817},
adsurl = {http://adsabs.harvard.edu/abs/1976ApJ...210..184E},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@book{Maeder:2009,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009pfer.book.....M},
author = {{Maeder}, A.},
booktitle = {Physics, Formation and Evolution of Rotating Stars: , Astronomy and Astrophysics Library.~ISBN 978-3-540-76948-4.~Springer Berlin Heidelberg, 2009},
doi = {10.1007/978-3-540-76949-1},
keywords = {Physics, Astrophysics, Astronomy},
publisher = {Springer-Verlag, Berlin},
title = {{Physics, Formation and Evolution of Rotating Stars}},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1007/978-3-540-76949-1},
}
@ARTICLE{Braithwaite:2006,
author = {{Braithwaite}, J.},
title = {{A differential rotation driven dynamo in a stably stratified star}},
journal = {\aap},
eprint = {arXiv:astro-ph/0509693},
keywords = {magnetohydrodynamics (MHD), stars: magnetic fields, stars: rotation, stars: evolution, Sun: rotation, instabilities},
year = {2006},
month = {apr},
volume = {449},
pages = {451-460},
doi = {10.1051/0004-6361:20054241},
adsurl = {http://adsabs.harvard.edu/abs/2006A%26A...449..451B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Zahn:2007,
author = {{Zahn}, J.-P. and {Brun}, A.~S. and {Mathis}, S.},
title = {{On magnetic instabilities and dynamo action in stellar radiation zones}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {0707.3287},
keywords = {instabilities, stars: magnetic fields, stars: rotation, magnetohydrodynamics (MHD)},
year = {2007},
month = {oct},
volume = {474},
pages = {145-154},
doi = {10.1051/0004-6361:20077653},
adsurl = {http://adsabs.harvard.edu/abs/2007A%26A...474..145Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Denissenkov:2010,
author = {{Denissenkov}, P.~A. and {Pinsonneault}, M. and {Terndrup}, D.~M. and {Newsham}, G.},
title = {{Angular Momentum Transport in Solar-type Stars: Testing the Timescale for Core-Envelope Coupling}},
journal = {\apj},
archiveprefix = {arXiv},
eprint = {0911.1121},
primaryclass = {astro-ph.SR},
keywords = {stars: evolution, stars: interiors, Sun: rotation},
year = {2010},
month = {jun},
volume = {716},
pages = {1269-1287},
doi = {10.1088/0004-637X/716/2/1269},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...716.1269D},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Zahn:1992,
author = {{Zahn}, J.-P.},
title = {{Circulation and turbulence in rotating stars}},
journal = {\aap},
keywords = {MERIDIONAL FLOW, STELLAR INTERIORS, STELLAR PHYSICS, STELLAR ROTATION, TURBULENCE, ANGULAR MOMENTUM, MOMENTUM TRANSFER, STELLAR COMPOSITION, STELLAR MODELS},
year = {1992},
month = {nov},
volume = {265},
pages = {115-132},
adsurl = {http://adsabs.harvard.edu/abs/1992A%26A...265..115Z},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Maeder:2000,
author = {{Maeder}, A. and {Meynet}, G.},
title = {{The Evolution of Rotating Stars}},
journal = {\araa},
eprint = {arXiv:astro-ph/0004204},
keywords = {STELLAR ROTATION, STELLAR EVOLUTION, MASS LOSS, MIXING, CHEMICAL ABUNDANCES},
year = {2000},
volume = {38},
pages = {143-190},
doi = {10.1146/annurev.astro.38.1.143},
adsurl = {http://adsabs.harvard.edu/abs/2000ARA%26A..38..143M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Maeder2012,
author = {{Maeder}, A. and {Meynet}, G.},
title = {{Rotating massive stars: From first stars to gamma ray bursts}},
journal = {Reviews of Modern Physics},
keywords = {Stellar rotation, Mass loss and stellar winds, Abundances, chemical composition, Main-sequence: early-type stars},
year = {2012},
month = {jan},
volume = {84},
pages = {25-63},
doi = {10.1103/RevModPhys.84.25},
adsurl = {http://adsabs.harvard.edu/abs/2012RvMP...84...25M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Langer2012,
author = {{Langer}, N.},
title = {{Presupernova Evolution of Massive Single and Binary Stars}},
journal = {\araa},
archiveprefix = {arXiv},
eprint = {1206.5443},
primaryclass = {astro-ph.SR},
year = {2012},
month = {sep},
volume = {50},
pages = {107-164},
doi = {10.1146/annurev-astro-081811-125534},
adsurl = {http://adsabs.harvard.edu/abs/2012ARA%26A..50..107L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@BOOK{Maeder2009,
author = {{Maeder}, A.},
title = {{Physics, Formation and Evolution of Rotating Stars}},
keywords = {Physics, Astrophysics, Astronomy},
booktitle = {Physics, Formation and Evolution of Rotating Stars: , Astronomy and Astrophysics Library.~ISBN 978-3-540-76948-4.~Springer Berlin Heidelberg, 2009},
year = {2009},
doi = {10.1007/978-3-540-76949-1},
adsurl = {http://adsabs.harvard.edu/abs/2009pfer.book.....M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Meynet2000,
author = {{Meynet}, G. and {Maeder}, A.},
title = {{Stellar evolution with rotation. V. Changes in all the outputs of massive star models}},
journal = {\aap},
eprint = {arXiv:astro-ph/0006404},
keywords = {STARS: ROTATION, STARS: EVOLUTION, STARS: ABUNDANCES, STARS: EARLY-TYPE},
year = {2000},
month = {sep},
volume = {361},
pages = {101-120},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...361..101M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Paxton:2011,
author = {{Paxton}, B. and {Bildsten}, L. and {Dotter}, A. and {Herwig}, F. and {Lesaffre}, P. and {Timmes}, F.},
title = {{Modules for Experiments in Stellar Astrophysics (MESA)}},
journal = {\apjs},
archiveprefix = {arXiv},
eprint = {1009.1622},
primaryclass = {astro-ph.SR},
keywords = {methods: numerical, stars: evolution, stars: general},
year = {2011},
month = {jan},
volume = {192},
eid = {3},
pages = {3},
doi = {10.1088/0067-0049/192/1/3},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJS..192....3P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Paxton:2013,
author = {{Paxton}, B. and {Cantiello}, M. and {Arras}, P. and {Bildsten}, L. and
{Brown}, E.~F. and {Dotter}, A. and {Mankovich}, C. and {Montgomery}, M.~H. and
{Stello}, D. and {Timmes}, F.~X. and {Townsend}, R.},
title = "{Modules for Experiments in Stellar Astrophysics (MESA): Planets, Oscillations, Rotation, and Massive Stars}",
journal = {\apjs},
archivePrefix = "arXiv",
eprint = {1301.0319},
primaryClass = "astro-ph.SR",
keywords = {asteroseismology, methods: numerical, planets and satellites: physical evolution, stars: evolution, stars: massive, stars: rotation},
year = 2013,
month = sep,
volume = 208,
eid = {4},
pages = {4},
doi = {10.1088/0067-0049/208/1/4},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJS..208....4P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System}
}
@ARTICLE{Heger:2000,
author = {{Heger}, A. and {Langer}, N. and {Woosley}, S.~E.},
title = {{Presupernova Evolution of Rotating Massive Stars. I. Numerical Method and Evolution of the Internal Stellar Structure}},
journal = {\apj},
eprint = {arXiv:astro-ph/9904132},
keywords = {HYDRODYNAMICS, METHODS: NUMERICAL, STARS EARLY-TYPE, STARS: EVOLUTION, STARS: INTERIORS, STARS ROTATION},
year = {2000},
month = {jan},
volume = {528},
pages = {368-396},
doi = {10.1086/308158},
adsurl = {http://adsabs.harvard.edu/abs/2000ApJ...528..368H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Heger:2005,
author = {{Heger}, A. and {Woosley}, S.~E. and {Spruit}, H.~C.},
title = {{Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields}},
journal = {\apj},
eprint = {arXiv:astro-ph/0409422},
keywords = {Stars: Pulsars: General, Stars: Evolution, Stars: Magnetic Fields, Stars: Rotation},
year = {2005},
month = {jun},
volume = {626},
pages = {350-363},
doi = {10.1086/429868},
adsurl = {http://adsabs.harvard.edu/abs/2005ApJ...626..350H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Spruit:1999,
author = {{Spruit}, H.~C.},
title = {{Differential rotation and magnetic fields in stellar interiors}},
journal = {\aap},
eprint = {arXiv:astro-ph/9907138},
keywords = {INSTABILITIES, MAGNETOHYDRODYNAMICS (MHD), STARS: MAGNETIC FIELDS, STARS: ROTATION, SUN: ROTATION},
year = {1999},
month = {sep},
volume = {349},
pages = {189-202},
adsurl = {http://adsabs.harvard.edu/abs/1999A%26A...349..189S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Spruit:2002,
author = {{Spruit}, H.~C.},
title = {{Dynamo action by differential rotation in a stably stratified stellar interior}},
journal = {\aap},
eprint = {arXiv:astro-ph/0108207},
keywords = {MAGNETOHYDRODYNAMICS (MHD), STARS: MAGNETIC FIELDS, INSTABILITIES},
year = {2002},
month = {jan},
volume = {381},
pages = {923-932},
doi = {10.1051/0004-6361:20011465},
adsurl = {http://adsabs.harvard.edu/abs/2002A%26A...381..923S},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{Petrovic:2005,
author = {{Petrovic}, J. and {Langer}, N. and {Yoon}, S.-C. and {Heger}, A.},
title = {{Which massive stars are gamma-ray burst progenitors?}},
journal = {\aap},
eprint = {arXiv:astro-ph/0504175},
keywords = {stars: evolution, stars: binaries: close, gamma rays: bursts, stars: rotation, stars: magnetic fields},
year = {2005},
month = {may},
volume = {435},
pages = {247-259},
doi = {10.1051/0004-6361:20042545},
adsurl = {http://adsabs.harvard.edu/abs/2005A%26A...435..247P},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{2010A&A...521A...9C,
author = {{Cantiello}, M. and {Langer}, N.},
title = {{Thermohaline mixing in evolved low-mass stars}},
journal = {\aap},
archiveprefix = {arXiv},
eprint = {1006.1354},
primaryclass = {astro-ph.SR},
keywords = {stars: abundances, stars: evolution, stars: magnetic field, nuclear reactions, nucleosynthesis, abundances, stars: AGB and post-AGB, stars: rotation},
year = {2010},
month = {oct},
volume = {521},
eid = {A9},
pages = {A9},
doi = {10.1051/0004-6361/201014305},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...521A...9C},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{2011ApJ...741...51R,
author = {{Robinson}, T.~D.},
title = {{Modeling the Infrared Spectrum of the Earth-Moon System: Implications for the Detection and Characterization of Earthlike Extrasolar Planets and Their Moonlike Companions}},
journal = {\apj},
archiveprefix = {arXiv},
eprint = {1110.3744},
primaryclass = {astro-ph.EP},
keywords = {astrobiology, Earth, infrared: planetary systems, Moon, planets and satellites: detection, techniques: miscellaneous},
year = {2011},
month = {nov},
volume = {741},
eid = {51},
pages = {51},
doi = {10.1088/0004-637X/741/1/51},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...741...51R},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@INPROCEEDINGS{2011AAS...21731805M,
author = {{Musielak}, D. and {Musielak}, Z.~E.},
title = {{Detection of Moons around Giant Extrasolar Planets}},
booktitle = {American Astronomical Society Meeting Abstracts \#217},
year = {2011},
series = {Bulletin of the American Astronomical Society},
volume = {43},
month = {jan},
pages = {#318.05},
adsurl = {http://adsabs.harvard.edu/abs/2011AAS...21731805M},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@ARTICLE{2008ApJ...685L.153L,
author = {{Lewis}, K.~M. and {Sackett}, P.~D. and {Mardling}, R.~A.},
title = {{Possibility of Detecting Moons of Pulsar Planets through Time-of-Arrival Analysis}},
journal = {\apjl},
archiveprefix = {arXiv},
eprint = {0805.4263},
keywords = {Stars: Planetary Systems, Stars: Pulsars: General, Stars: Pulsars: Individual: Alphanumeric: PSR B1620-26, Stars: Oscillations},
year = {2008},
month = {oct},
volume = {685},
pages = {L153-L156},
doi = {10.1086/592743},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...685L.153L},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@article{lo_Langer_Pols_Brott_Yoon_2009,
title = {{Rotational mixing in massive binaries}},
volume = {497},
url = {http://dx.doi.org/10.1051/0004-6361/200811439},
doi = {10.1051/0004-6361/200811439},
number = {1},
journal = {Astronomy and Astrophysics},
publisher = {EDP Sciences},
author = {de Mink, S. E. and Cantiello, M. and Langer, N. and Pols, O. R. and Brott, I. and Yoon, S.-Ch.},
year = {2009},
month = {Apr},
pages = {243-253},
}
@article{larends_Yoon_Heger_Herwig_2008,
title = {{White dwarf spins from low-mass stellar evolution models}},
volume = {481},
url = {http://dx.doi.org/10.1051/0004-6361:200809411},
doi = {10.1051/0004-6361:200809411},
number = {3},
journal = {Astronomy and Astrophysics},
publisher = {EDP Sciences},
author = {Suijs, M. P. L. and Langer, N. and Poelarends, A.-J. and Yoon, S.-C. and Heger, A. and Herwig, F.},
year = {2008},
month = {Apr},
pages = {L87-L90},
}
@article{Heger_Langer_Woosley_2000,
title = {{Presupernova Evolution of Rotating Massive Stars. I. Numerical Method and Evolution of the Internal Stellar Structure}},
volume = {528},
url = {http://dx.doi.org/10.1086/308158},
doi = {10.1086/308158},
number = {1},
journal = {The Astrophysical Journal},
publisher = {IOP Publishing},
author = {Heger, A. and Langer, N. and Woosley, S. E.},
year = {2000},
month = {Jan},
pages = {368-396},
}
@book{Maeder_2009,
title = {{The evolution of AGB stars with convective overshoot}},
isbn = {978-3-540-76948-4},
url = {http://dx.doi.org/10.1007/978-3-540-76949-1_10},
doi = {10.1007/978-3-540-76949-1_10},
publisher = {Springer-Verlag},
author = {{Herwig}, F.},
year = {2000},
pages = {952-968},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...360..952H},
eprint = {arXiv:astro-ph/0007139},
journal = {\aap},
keywords = {STARS: ABUNDANCES, STARS: INTERIORS, STARS: EVOLUTION, STARS: AGB AND POST-AGB},
month = {aug},
volume = {360},
}
@inproceedings{augustson11b,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011IAUS..271..361A},
archiveprefix = {arXiv},
author = {{Augustson}, K.~C. and {Brun}, A.~S. and {Toomre}, J.},
booktitle = {Proc. IAU Symp. 271},
doi = {10.1017/S1743921311017790},
editor = {{Brummell}, N.~H. and {Brun}, A.~S. and {Miesch}, M.~S. and {Ponty}, Y.},
eprint = {1011.1016},
keywords = {stars: early type, rotation, magnetic fields},
month = {aug},
pages = {361-362},
primaryclass = {astro-ph.SR},
title = {{Convection and dynamo action in B stars}},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1017/S1743921311017790},
}
@article{lee93,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1993MNRAS.261..415L},
author = {{Lee}, U. and {Saio}, H.},
journal = {\mnras},
keywords = {ANGULAR MOMENTUM, MASSIVE STARS, MOMENTUM TRANSFER, STELLAR OSCILLATIONS, STELLAR PHYSICS, STELLAR ROTATION, MAIN SEQUENCE STARS, REYNOLDS STRESS, STELLAR MODELS},
month = {mar},
pages = {415-424},
title = {{Angular momentum transfer by non-radial oscillations in massive main-sequence stars}},
volume = {261},
year = {1993},
}
@article{featherstone09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...705.1000F},
author = {{Featherstone}, N.~A. and {Browning}, M.~K. and {Brun}, A.~S. and {Toomre}, J.},
doi = {10.1088/0004-637X/705/1/1000},
journal = {\apj},
keywords = {convection, MHD, stars: evolution, stars: interiors, stars: magnetic fields},
month = {nov},
pages = {1000-1018},
title = {{Effects of Fossil Magnetic Fields on Convective Core Dynamos in A-type Stars}},
volume = {705},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/705/1/1000},
}
@inproceedings{toomre11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011IAUS..271..347T},
author = {{Toomre}, J.},
booktitle = {Proc. IAU Symp. 271},
doi = {10.1017/S1743921311017777},
editor = {{Brummell}, N.~H. and {Brun}, A.~S. and {Miesch}, M.~S. and {Ponty}, Y.},
keywords = {Sun: tachocline, Sun: near-surface shear layer, Sun: dynamo action, stars: massive star convection},
month = {aug},
pages = {347-352},
title = {{Onward from solar convection to dynamos in cores of massive stars}},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1017/S1743921311017777},
}
@article{2013A&A...549A..74M,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2013A%26A...549A..74M},
archiveprefix = {arXiv},
author = {{Marques}, J.~P. and {Goupil}, M.~J. and {Lebreton}, Y. and {Talon}, S. and {Palacios}, A. and {Belkacem}, K. and {Ouazzani}, R.-M. and {Mosser}, B. and {Moya}, A. and {Morel}, P. and {Pichon}, B. and {Mathis}, S. and {Zahn}, J.-P. and {Turck-Chi{\`e}ze}, S. and {Nghiem}, P.~A.~P.},
doi = {10.1051/0004-6361/201220211},
eid = {A74},
eprint = {1211.1271},
journal = {\aap},
keywords = {stars: evolution, stars: interiors, stars: rotation, stars: oscillations},
month = {jan},
pages = {A74, 15pp},
primaryclass = {astro-ph.SR},
title = {{Seismic diagnostics for transport of angular momentum in stars. I. Rotational splittings from the pre-main sequence to the red-giant branch}},
volume = {549},
year = {2013},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201220211},
}
@article{2012Natur.481...55B,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012Natur.481...55B},
archiveprefix = {arXiv},
author = {{Beck}, P.~G. and {Montalban}, J. and {Kallinger}, T. and {De Ridder}, J. and {Aerts}, C. and {Garc{\'{\i}}a}, R.~A. and {Hekker}, S. and {Dupret}, M.-A. and {Mosser}, B. and {Eggenberger}, P. and {Stello}, D. and {Elsworth}, Y. and {Frandsen}, S. and {Carrier}, F. and {Hillen}, M. and {Gruberbauer}, M. and {Christensen-Dalsgaard}, J. and {Miglio}, A. and {Valentini}, M. and {Bedding}, T.~R. and {Kjeldsen}, H. and {Girouard}, F.~R. and {Hall}, J.~R. and {Ibrahim}, K.~A.},
doi = {10.1038/nature10612},
eprint = {1112.2825},
journal = {\nat},
month = {jan},
pages = {55-57},
primaryclass = {astro-ph.SR},
title = {{Fast core rotation in red-giant stars as revealed by gravity-dominated mixed modes}},
volume = {481},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature10612},
}
@article{meneveau00,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000AnRFM..32....1M},
author = {{Meneveau}, C. and {Katz}, J.},
doi = {10.1146/annurev.fluid.32.1.1},
journal = {\arfm},
pages = {1-32},
title = {{Scale-Invariance and Turbulence Models for Large-Eddy Simulation}},
volume = {32},
year = {2000},
bdsk-url-1 = {http://dx.doi.org/10.1146/annurev.fluid.32.1.1},
}
@article{rempel09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...691..640R},
archiveprefix = {arXiv},
author = {{Rempel}, M. and {Sch{\"u}ssler}, M. and {Kn{\"o}lker}, M.},
doi = {10.1088/0004-637X/691/1/640},
eprint = {0808.3294},
journal = {\apj},
keywords = {convection, MHD, radiative transfer, sunspots},
month = {jan},
pages = {640-649},
title = {{Radiative Magnetohydrodynamic Simulation of Sunspot Structure}},
volume = {691},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/691/1/640},
}
@article{stello13,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2013arXiv1302.0858S},
archiveprefix = {arXiv},
author = {{Stello}, D. and {Huber}, D. and {Bedding}, T.~R. and {Benomar}, O. and {Bildsten}, L. and {Elsworth}, Y.~P. and {Gilliland}, R.~L. and {Mosser}, B. and {Paxton}, B. and {White}, T.~R.},
eprint = {1302.0858},
journal = {\arXiv:1302.0858},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {feb},
primaryclass = {astro-ph.SR},
title = {{Asteroseismic classification of stellar populations among 13000 red giants observed by Kepler}},
year = {2013},
}
@article{Clune:1999,
author = {{Clune}, T.~C. and {Elliott}, J.~R. and {Miesch}, M.~S. and {Toomre}, J.},
journal = {\parcomp},
pages = {361-380},
volume = {25},
title = {{Computational aspects of a code to study rotating turbulent convection in spherical shells}},
year = {1999},
}
@article{Ofek:2013,
author = {{Ofek}, E.~O. and {Sullivan}, M. and {Cenko}, S.B. and {Kasliwal}, M.M. and {Gal-Yam}, A. and {Kulkarni}, S.R and {Arcavi}, I. and {Bildsten}, L. and {Bloom}, J.S. and {Horesh}, A. and {Howell}, D.A. and {Filippenko}, A.V. and {Laher}, R. and {Murray}, D. and {Nakar}, E. and {Nugent}, P.E. and {Silverman}, J.M and {Shaviv}, N.J. and {Surace}, J. and {Yaron}, O.},
doi = {10.1038/nature11877},
journal = {\nat},
month = {feb},
pages = {65-67},
title = {{An outburst from a massive star 40 days before a supernova explosion}},
volume = {494},
year = {2013},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature11877},
}
@article{Christensen-Dalsgaard:2008,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008Ap%26SS.316..113C},
archiveprefix = {arXiv},
author = {{Christensen-Dalsgaard}, J.},
doi = {10.1007/s10509-007-9689-z},
eprint = {0710.3106},
journal = {\apss},
keywords = {Stars: oscillations, Numerical methods, Asteroseismology},
month = {aug},
pages = {113-120},
title = {{ADIPLS --- the Aarhus adiabatic oscillation package}},
volume = {316},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1007/s10509-007-9689-z},
}
@article{Brun:2004,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2004ApJ...614.1073B},
author = {{Brun}, A.~S. and {Miesch}, M.~S. and {Toomre}, J.},
doi = {10.1086/423835},
eprint = {arXiv:astro-ph/0610073},
journal = {\apj},
keywords = {Convection, Magnetohydrodynamics: MHD, Sun: Magnetic Fields, Turbulence},
month = {oct},
pages = {1073-1098},
title = {{Global-Scale Turbulent Convection and Magnetic Dynamo Action in the Solar Envelope}},
volume = {614},
year = {2004},
bdsk-url-1 = {http://dx.doi.org/10.1086/423835},
}
@article{Augustson:2011,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011JPhCS.271a2070A},
archiveprefix = {arXiv},
author = {{Augustson}, K. and {Rast}, M. and {Trampedach}, R. and {Toomre}, J.},
doi = {10.1088/1742-6596/271/1/012070},
eprint = {1012.4781},
journal = {J. Phys. Conf. Ser. 271},
month = {jan},
number = {1},
pages = {012070, 4pp},
primaryclass = {astro-ph.SR},
title = {{Modeling the Near-Surface Shear Layer: Diffusion Schemes Studied With CSS}},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/1742-6596/271/1/012070},
}
@article{Brott:2011,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011A%26A...530A.116B},
archiveprefix = {arXiv},
author = {{Brott}, I. and {Evans}, C.~J. and {Hunter}, I. and {de Koter}, A. and {Langer}, N. and {Dufton}, P.~L. and {Cantiello}, M. and {Trundle}, C. and {Lennon}, D.~J. and {de Mink}, S.~E. and {Yoon}, S.-C. and {Anders}, P.},
doi = {10.1051/0004-6361/201016114},
eid = {A116},
eprint = {1102.0766},
journal = {\aap},
keywords = {methods: statistical, stars: abundances, stars: evolution, stars: early-type, stars: massive, stars: rotation},
month = {jun},
pages = {A116, 17pp},
primaryclass = {astro-ph.SR},
title = {{Rotating massive main-sequence stars. II. Simulating a population of LMC early B-type stars as a test of rotational mixing}},
volume = {530},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201016114},
}
@article{Poelarends:2008,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...675..614P},
archiveprefix = {arXiv},
author = {{Poelarends}, A.~J.~T. and {Herwig}, F. and {Langer}, N. and {Heger}, A.},
doi = {10.1086/520872},
eprint = {0705.4643},
journal = {\apj},
keywords = {Stars: AGB and Post-AGB, Stars: Evolution, Stars: Neutron, Stars: Supernovae: General},
month = {mar},
pages = {614-625},
title = {{The Supernova Channel of Super-AGB Stars}},
volume = {675},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1086/520872},
}
@article{Kochanek:2011,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...741...37K},
archiveprefix = {arXiv},
author = {{Kochanek}, C.~S.},
doi = {10.1088/0004-637X/741/1/37},
eid = {37},
eprint = {1106.4722},
journal = {\apj},
keywords = {stars: evolution, supergiants, supernovae: general, supernovae: individual: SN 2008S 2008 NGC 300-OT},
month = {nov},
pages = {37, 17pp},
primaryclass = {astro-ph.SR},
title = {{Dusty Explosions from Dusty Progenitors: The Physics of SN 2008S and the 2008 NGC 300-OT}},
volume = {741},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/741/1/37},
}
@article{Thompson:2009,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...705.1364T},
archiveprefix = {arXiv},
author = {{Thompson}, T.~A. and {Prieto}, J.~L. and {Stanek}, K.~Z. and {Kistler}, M.~D. and {Beacom}, J.~F. and {Kochanek}, C.~S.},
doi = {10.1088/0004-637X/705/2/1364},
eprint = {0809.0510},
journal = {\apj},
keywords = {stars: evolution, supernovae: general, supernovae: individual: SN 2008S 1999bw, surveys},
month = {nov},
pages = {1364-1384},
title = {{A New Class of Luminous Transients and a First Census of their Massive Stellar Progenitors}},
volume = {705},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/705/2/1364},
}
@article{Arcavi:2012,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...756L..30A},
archiveprefix = {arXiv},
author = {{Arcavi}, I. and {Gal-Yam}, A. and {Cenko}, S.~B. and {Fox}, D.~B. and {Leonard}, D.~C. and {Moon}, D.-S. and {Sand}, D.~J. and {Soderberg}, A.~M. and {Kiewe}, M. and {Yaron}, O. and {Becker}, A.~B. and {Scheps}, R. and {Birenbaum}, G. and {Chamudot}, D. and {Zhou}, J.},
doi = {10.1088/2041-8205/756/2/L30},
eid = {L30},
eprint = {1206.2029},
journal = {\apjl},
keywords = {supernovae: general},
month = {sep},
pages = {L30, 6pp},
primaryclass = {astro-ph.CO},
title = {{Caltech Core-Collapse Project (CCCP) Observations of Type II Supernovae: Evidence for Three Distinct Photometric Subtypes}},
volume = {756},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/756/2/L30},
}
@article{Yoon:2010,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...717L..62Y},
archiveprefix = {arXiv},
author = {{Yoon}, S.-C. and {Cantiello}, M.},
doi = {10.1088/2041-8205/717/1/L62},
eprint = {1005.4925},
journal = {\apjl},
keywords = {stars: evolution, stars: massive, stars: mass-loss, supergiants, supernovae: general},
month = {jul},
pages = {L62-L65},
primaryclass = {astro-ph.SR},
title = {{Evolution of Massive Stars with Pulsation-driven Superwinds During the Red Supergiant Phase}},
volume = {717},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/717/1/L62},
}
@article{Woosley:2010,
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adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...719L.204W},
archiveprefix = {arXiv},
author = {{Woosley}, S.~E.},
doi = {10.1088/2041-8205/719/2/L204},
eprint = {0911.0698},
journal = {\apjl},
keywords = {hydrodynamics, shock waves, supernovae: general, turbulence},
month = {aug},
pages = {L204-L207},
primaryclass = {astro-ph.HE},
title = {{Bright Supernovae from Magnetar Birth}},
volume = {719},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/719/2/L204},
}
@article{Kalirai:2008,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...676..594K},
archiveprefix = {arXiv},
author = {{Kalirai}, J.~S. and {Hansen}, B.~M.~S. and {Kelson}, D.~D. and {Reitzel}, D.~B. and {Rich}, R.~M. and {Richer}, H.~B.},
doi = {10.1086/527028},
eprint = {0706.3894},
journal = {\apj},
keywords = {open clusters and associations: individual (NGC 6819), open clusters and associations: individual (NGC 7789), Stars: Evolution, Techniques: Photometric, Techniques: Spectroscopic, Stars: White Dwarfs},
month = {mar},
pages = {594-609},
title = {{The Initial-Final Mass Relation: Direct Constraints at the Low-Mass End}},
volume = {676},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1086/527028},
}
@article{Gal-Yam:2012,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012Sci...337..927G},
archiveprefix = {arXiv},
author = {{Gal-Yam}, A.},
doi = {10.1126/science.1203601},
eprint = {1208.3217},
journal = {\sci},
month = {aug},
pages = {927-932},
primaryclass = {astro-ph.CO},
title = {{Luminous Supernovae}},
volume = {337},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1126/science.1203601},
}
@article{Quataert:2012,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.423L..92Q},
archiveprefix = {arXiv},
author = {{Quataert}, E. and {Shiode}, J.},
doi = {10.1111/j.1745-3933.2012.01264.x},
eprint = {1202.5036},
journal = {\mnras},
keywords = {stars: mass loss, supernovae: general},
month = {jun},
pages = {L92-L96},
primaryclass = {astro-ph.SR},
title = {{Wave-driven mass loss in the last year of stellar evolution: setting the stage for the most luminous core-collapse supernovae}},
volume = {423},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1745-3933.2012.01264.x},
}
@article{Chomiuk:2011,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...743..114C},
archiveprefix = {arXiv},
author = {{Chomiuk}, L. and {Chornock}, R. and {Soderberg}, A.~M. and {Berger}, E. and {Chevalier}, R.~A. and {Foley}, R.~J. and {Huber}, M.~E. and {Narayan}, G. and {Rest}, A. and {Gezari}, S. and {Kirshner}, R.~P. and {Riess}, A. and {Rodney}, S.~A. and {Smartt}, S.~J. and {Stubbs}, C.~W. and {Tonry}, J.~L. and {Wood-Vasey}, W.~M. and {Burgett}, W.~S. and {Chambers}, K.~C. and {Czekala}, I. and {Flewelling}, H. and {Forster}, K. and {Kaiser}, N. and {Kudritzki}, R.-P. and {Magnier}, E.~A. and {Martin}, D.~C. and {Morgan}, J.~S. and {Neill}, J.~D. and {Price}, P.~A. and {Roth}, K.~C. and {Sanders}, N.~E. and {Wainscoat}, R.~J.},
doi = {10.1088/0004-637X/743/2/114},
eid = {114},
eprint = {1107.3552},
journal = {\apj},
keywords = {circumstellar matter, stars: magnetars, supernovae: general, supernovae: individual: PS1-10ky PS1-10awh},
month = {dec},
pages = {114, 19pp},
primaryclass = {astro-ph.HE},
title = {{Pan-STARRS1 Discovery of Two Ultraluminous Supernovae at z$\sim$0.9}},
volume = {743},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/743/2/114},
}
@article{Quimby:2011,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011Natur.474..487Q},
archiveprefix = {arXiv},
author = {{Quimby}, R.~M. and {Kulkarni}, S.~R. and {Kasliwal}, M.~M. and {Gal-Yam}, A. and {Arcavi}, I. and {Sullivan}, M. and {Nugent}, P. and {Thomas}, R. and {Howell}, D.~A. and {Nakar}, E. and {Bildsten}, L. and {Theissen}, C. and {Law}, N.~M. and {Dekany}, R. and {Rahmer}, G. and {Hale}, D. and {Smith}, R. and {Ofek}, E.~O. and {Zolkower}, J. and {Velur}, V. and {Walters}, R. and {Henning}, J. and {Bui}, K. and {McKenna}, D. and {Poznanski}, D. and {Cenko}, S.~B. and {Levitan}, D.},
doi = {10.1038/nature10095},
eprint = {0910.0059},
journal = {\nat},
month = {jun},
pages = {487-489},
primaryclass = {astro-ph.CO},
title = {{Hydrogen-poor superluminous stellar explosions}},
volume = {474},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature10095},
}
@article{Smith:2011,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011MNRAS.412.1522S},
archiveprefix = {arXiv},
author = {{Smith}, N. and {Li}, W. and {Filippenko}, A.~V. and {Chornock}, R.},
doi = {10.1111/j.1365-2966.2011.17229.x},
eprint = {1006.3899},
journal = {\mnras},
keywords = {binaries: general, stars: evolution, stars: mass-loss, supernovae: general},
month = {apr},
pages = {1522-1538},
primaryclass = {astro-ph.HE},
title = {{Observed fractions of core-collapse supernova types and initial masses of their single and binary progenitor stars}},
volume = {412},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2011.17229.x},
}
@article{Kasen:2010,
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adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...717..245K},
archiveprefix = {arXiv},
author = {{Kasen}, D. and {Bildsten}, L.},
doi = {10.1088/0004-637X/717/1/245},
eprint = {0911.0680},
journal = {\apj},
keywords = {radiative transfer, stars: neutron, supernovae: general, supernovae: individual: SN 2005ap SN 2008es SN 2007bi},
month = {jul},
pages = {245-249},
primaryclass = {astro-ph.HE},
title = {{Supernova Light Curves Powered by Young Magnetars}},
volume = {717},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/717/1/245},
}
@article{Gal-Yam:2009,
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adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...705.1364T},
archiveprefix = {arXiv},
author = {{Thompson}, T.~A. and {Prieto}, J.~L. and {Stanek}, K.~Z. and {Kistler}, M.~D. and {Beacom}, J.~F. and {Kochanek}, C.~S.},
doi = {10.1088/0004-637X/705/2/1364},
eprint = {0809.0510},
journal = {\apj},
keywords = {stars: evolution, supernovae: general, supernovae: individual: SN 2008S 1999bw, surveys},
month = {nov},
pages = {1364-1384},
title = {{A New Class of Luminous Transients and a First Census of their Massive Stellar Progenitors}},
volume = {705},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/705/2/1364},
}
@article{Smartt:2009,
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adsurl = {http://adsabs.harvard.edu/abs/2009MNRAS.395.1409S},
archiveprefix = {arXiv},
author = {{Smartt}, S.~J. and {Eldridge}, J.~J. and {Crockett}, R.~M. and {Maund}, J.~R.},
doi = {10.1111/j.1365-2966.2009.14506.x},
eprint = {0809.0403},
journal = {\mnras},
keywords = {stars: evolution , supergiants , supernovae: general , galaxies: stellar content},
month = {may},
pages = {1409-1437},
title = {{The death of massive stars - I. Observational constraints on the progenitors of Type II-P supernovae}},
volume = {395},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2009.14506.x},
}
@article{Smartt:2009b,
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adsurl = {http://adsabs.harvard.edu/abs/2009ARA%26A..47...63S},
archiveprefix = {arXiv},
author = {{Smartt}, S.~J.},
doi = {10.1146/annurev-astro-082708-101737},
eprint = {0908.0700},
journal = {\araa},
month = {sep},
pages = {63-106},
primaryclass = {astro-ph.SR},
title = {{Progenitors of Core-Collapse Supernovae}},
volume = {47},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1146/annurev-astro-082708-101737},
}
@article{2008ApJ...681L...9P,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...675..614P},
author = {{Prieto}, J.~L. and {Kistler}, M.~D. and {Thompson}, T.~A. and and {Hansen}, B.~M.~S. and {Kelson}, D.~D. and ars: Supernovae: General},
doi = {10.1086/520872},
month = {mar},
pages = {614-625},
volume = {675},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1086/520872},
}
@article{Ofek:2007,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2007ApJ...659L..13O},
author = {{Ofek}, E.~O. and {Cameron}, P.~B. and {Kasliwal}, M.~M. and {Gal-Yam}, A. and {Rau}, A. and {Kulkarni}, S.~R. and {Frail}, D.~A. and {Chandra}, P. and {Cenko}, S.~B. and {Soderberg}, A.~M. and {Immler}, S.},
doi = {10.1086/516749},
eprint = {arXiv:astro-ph/0612408},
journal = {\apjl},
keywords = {galaxies: individual (NGC 1260), Stars: Supernovae: General, supernovae: individual (SN 2006gy)},
month = {apr},
pages = {L13-L16},
title = {{SN 2006gy: An Extremely Luminous Supernova in the Galaxy NGC 1260}},
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year = {2007},
bdsk-url-1 = {http://dx.doi.org/10.1086/516749},
}
@article{Smith:2007,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2007ApJ...666.1116S},
author = {{Smith}, N. and {Li}, W. and {Foley}, R.~J. and {Wheeler}, J.~C. and {Pooley}, D. and {Chornock}, R. and {Filippenko}, A.~V. and {Silverman}, J.~M. and {Quimby}, R. and {Bloom}, J.~S. and {Hansen}, C.},
doi = {10.1086/519949},
eprint = {arXiv:astro-ph/0612617},
journal = {\apj},
keywords = {Stars: Circumstellar Matter, Stars: Evolution, supernovae: individual (SN 2006gy)},
month = {sep},
pages = {1116-1128},
title = {{SN 2006gy: Discovery of the Most Luminous Supernova Ever Recorded, Powered by the Death of an Extremely Massive Star like {$\eta$} Carinae}},
volume = {666},
year = {2007},
bdsk-url-1 = {http://dx.doi.org/10.1086/519949},
}
@article{Smith:2007b,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2007ApJ...671L..17S},
archiveprefix = {arXiv},
author = {{Smith}, N. and {McCray}, R.},
doi = {10.1086/524681},
eprint = {0710.3428},
journal = {\apjl},
keywords = {Stars: Circumstellar Matter, Stars: Evolution, supernovae: individual (SN 2006gy)},
month = {dec},
pages = {L17-L20},
title = {{Shell-shocked Diffusion Model for the Light Curve of SN 2006gy}},
volume = {671},
year = {2007},
bdsk-url-1 = {http://dx.doi.org/10.1086/524681},
}
@article{2006A&A...450..345K,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2006A%26A...450..345K},
author = {{Kitaura}, F.~S. and {Janka}, H.-T. and {Hillebrandt}, W.},
doi = {10.1051/0004-6361:20054703},
eprint = {arXiv:astro-ph/0512065},
journal = {\aap},
keywords = {stars: supernovae: general, stars: supernovae: individual: Crab, neutrinos, hydrodynamics, radiative transfer},
month = {apr},
pages = {345-350},
title = {{Explosions of O-Ne-Mg cores, the Crab supernova, and subluminous type II-P supernovae}},
volume = {450},
year = {2006},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20054703},
}
@article{2006A&A...448..717S,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2006A%26A...448..717S},
author = {{Siess}, L.},
doi = {10.1051/0004-6361:20053043},
journal = {\aap},
keywords = {stars: evolution, nuclear reactions, nucleosynthesis, , abundances, stars: AGB and post-AGB},
month = {mar},
pages = {717-729},
title = {{Evolution of massive AGB stars. I. Carbon burning phase}},
volume = {448},
year = {2006},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20053043},
}
@article{1996ApJ...460..489R,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1996ApJ...460..489R},
author = {{Ritossa}, C. and {Garcia-Berro}, E. and {Iben}, Jr., I.},
doi = {10.1086/176987},
journal = {\apj},
keywords = {STARS: NOVAE, CATACLYSMIC VARIABLES, NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: ABUNDANCES, STARS: AGB AND POST-AGB, STARS: EVOLUTION, STARS: INTERIORS, STARS: VARIABLES: OTHER LONG-PERIOD VARIABLES},
month = {mar},
pages = {489-505},
title = {{On the Evolution of Stars That Form Electron-degenerate Cores Processed by Carbon Burning. II. Isotope Abundances and Thermal Pulses in a 10 M$_{sun}$ Model with an ONe Core and Applications to Long-Period Variables, Classical Novae, and Accretion-induced Collapse}},
volume = {460},
year = {1996},
bdsk-url-1 = {http://dx.doi.org/10.1086/176987},
}
@article{1987ApJ...322..206N,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1987ApJ...322..206N},
author = {{Nomoto}, K.},
doi = {10.1086/165716},
journal = {\apj},
keywords = {ELECTRON CAPTURE, GRAVITATIONAL COLLAPSE, STELLAR CORES, STELLAR EVOLUTION, STELLAR MASS, SUPERNOVAE, CRAB NEBULA, NUCLEAR FUSION, STELLAR INTERIORS, STELLAR MODELS},
month = {nov},
pages = {206-214},
title = {{Evolution of 8-10 solar mass stars toward electron capture supernovae. II - Collapse of an O + NE + MG core}},
volume = {322},
year = {1987},
bdsk-url-1 = {http://dx.doi.org/10.1086/165716},
}
@article{1984ApJ...277..791N,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1984ApJ...277..791N},
author = {{Nomoto}, K.},
doi = {10.1086/161749},
journal = {\apj},
keywords = {ABUNDANCE, ELECTRON CAPTURE, STELLAR EVOLUTION, STELLAR STRUCTURE, SUPERNOVAE, CARBON STARS, GRAVITATIONAL COLLAPSE, MAGNESIUM, MILKY WAY GALAXY, NEON, NUCLEAR FUSION, OXYGEN, WHITE DWARF STARS},
month = {feb},
pages = {791-805},
title = {{Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG cores}},
volume = {277},
year = {1984},
bdsk-url-1 = {http://dx.doi.org/10.1086/161749},
}
@article{MaeMey2000,
author = {{Maeder}, A. and {Meynet}, G.},
journal = {\araa},
pages = {143-190},
title = {{The Evolution of Rotating Stars}},
volume = {38},
year = {2000},
}
@article{Pan2007,
author = {{Pantillon}, F.~P. and {Talon}, S. and {Charbonnel}, C.},
journal = {\aap},
month = {oct},
pages = {155-163},
title = {{Angular momentum transport by internal gravity waves. III. Wave excitation by core convection and the Coriolis effect}},
volume = {474},
year = {2007},
}
@article{Mat2009,
author = {{Mathis}, S.},
journal = {\aap},
month = {nov},
pages = {811-828},
title = {{Transport by gravito-inertial waves in differentially rotating stellar radiation zones. I - Theoretical formulation}},
volume = {506},
year = {2009},
}
@book{aerts10,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010aste.book.....A},
author = {{Aerts}, C. and {Christensen-Dalsgaard}, J. and {Kurtz}, D.~W.},
booktitle = {Asteroseismology by C.~Aerts, J.~Christensen-Dalsgaard, and D.W.~Kurtz.~Springer, 2010.},
editor = {{Aerts, C., Christensen-Dalsgaard, J., \& Kurtz, D.~W.}},
title = {{Asteroseismology}},
year = {2010},
}
@article{aizenman77,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1977A%26A....58...41A},
author = {{Aizenman}, M. and {Smeyers}, P. and {Weigert}, A.},
journal = {\aap},
month = {jun},
pages = {41-46},
title = {{Avoided Crossing of Modes of Non-radial Stellar Oscillations}},
volume = {58},
year = {1977},
}
@inproceedings{baglin09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009IAUS..253...71B},
author = {{Baglin}, A. and {Auvergne}, M. and {Barge}, P. and {Deleuil}, M. and {Michel}, E. and {The CoRoT Exoplanet Science Team}},
booktitle = {Proc. IAU Symp. 253},
doi = {10.1017/S1743921308026252},
month = {feb},
pages = {71-81},
title = {{CoRoT: Description of the Mission and Early Results}},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1017/S1743921308026252},
}
@article{baudin11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011A%26A...529A..84B},
archiveprefix = {arXiv},
author = {{Baudin}, F. and {Barban}, C. and {Belkacem}, K. and {Hekker}, S. and {Morel}, T. and {Samadi}, R. and {Benomar}, O. and {Goupil}, M.-J. and {Carrier}, F. and {Ballot}, J. and {Deheuvels}, S. and {De Ridder}, J. and {Hatzes}, A.~P. and {Kallinger}, T. and {Weiss}, W.~W.},
doi = {10.1051/0004-6361/201014037},
eprint = {1102.1896},
journal = {\aap},
keywords = {asteroseismology, methods: data analysis, stars: oscillations},
month = {may},
pages = {A84, 8pp},
primaryclass = {astro-ph.SR},
title = {{Amplitudes and lifetimes of solar-like oscillations observed by CoRoT. Red-giant versus main-sequence stars}},
volume = {529},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201014037},
}
@article{beck11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011Sci...332..205B},
author = {{Beck}, P.~G. and {Bedding}, T.~R. and {Mosser}, B. and {Stello}, D. and {Garcia}, R.~A. and {Kallinger}, T. and {Hekker}, S. and {Elsworth}, Y. and {Frandsen}, S. and {Carrier}, F. and {De Ridder}, J. and {Aerts}, C. and {White}, T.~R. and {Huber}, D. and {Dupret}, M.-A. and {Montalb{\'a}n}, J. and {Miglio}, A. and {Noels}, A. and {Chaplin}, W.~J. and {Kjeldsen}, H. and {Christensen-Dalsgaard}, J. and {Gilliland}, R.~L. and {Brown}, T.~M. and {Kawaler}, S.~D. and {Mathur}, S. and {Jenkins}, J.~M.},
doi = {10.1126/science.1201939},
journal = {\sci},
month = {apr},
pages = {205},
title = {{Kepler Detected Gravity-Mode Period Spacings in a Red Giant Star}},
volume = {332},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1126/science.1201939},
}
@article{bedding10,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...713L.176B},
archiveprefix = {arXiv},
author = {{Bedding}, T.~R. and {Huber}, D. and {Stello}, D. and {Elsworth}, Y.~P. and {Hekker}, S. and {Kallinger}, T. and {Mathur}, S. and {Mosser}, B. and {Preston}, H.~L. and {Ballot}, J. and {Barban}, C. and {Broomhall}, A.~M. and {Buzasi}, D.~L. and {Chaplin}, W.~J. and {Garc{\'{\i}}a}, R.~A. and {Gruberbauer}, M. and {Hale}, S.~J. and {De Ridder}, J. and {Frandsen}, S. and {Borucki}, W.~J. and {Brown}, T. and {Christensen-Dalsgaard}, J. and {Gilliland}, R.~L. and {Jenkins}, J.~M. and {Kjeldsen}, H. and {Koch}, D. and {Belkacem}, K. and {Bildsten}, L. and {Bruntt}, H. and {Campante}, T.~L. and {Deheuvels}, S. and {Derekas}, A. and {Dupret}, M.-A. and {Goupil}, M.-J. and {Hatzes}, A. and {Houdek}, G. and {Ireland}, M.~J. and {Jiang}, C. and {Karoff}, C. and {Kiss}, L.~L. and {Lebreton}, Y. and {Miglio}, A. and {Montalb{\'a}n}, J. and {Noels}, A. and {Roxburgh}, I.~W. and {Sangaralingam}, V. and {Stevens}, I.~R. and {Suran}, M.~D. and {Tarrant}, N.~J. and {Weiss}, A.},
doi = {10.1088/2041-8205/713/2/L176},
eprint = {1001.0229},
journal = {\apjl},
keywords = {stars: oscillations},
month = {apr},
pages = {L176-L181},
primaryclass = {astro-ph.SR},
title = {{Solar-like Oscillations in Low-luminosity Red Giants: First Results from Kepler}},
volume = {713},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/713/2/L176},
}
@article{bedding11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011Natur.471..608B},
archiveprefix = {arXiv},
author = {{Bedding}, T.~R. and {Mosser}, B. and {Huber}, D. and {Montalb{\'a}n}, J. and {Beck}, P. and {Christensen-Dalsgaard}, J. and {Elsworth}, Y.~P. and {Garc{\'{\i}}a}, R.~A. and {Miglio}, A. and {Stello}, D. and {White}, T.~R. and {De Ridder}, J. and {Hekker}, S. and {Aerts}, C. and {Barban}, C. and {Belkacem}, K. and {Broomhall}, A.-M. and {Brown}, T.~M. and {Buzasi}, D.~L. and {Carrier}, F. and {Chaplin}, W.~J. and {di Mauro}, M.~P. and {Dupret}, M.-A. and {Frandsen}, S. and {Gilliland}, R.~L. and {Goupil}, M.-J. and {Jenkins}, J.~M. and {Kallinger}, T. and {Kawaler}, S. and {Kjeldsen}, H. and {Mathur}, S. and {Noels}, A. and {Aguirre}, V.~S. and {Ventura}, P.},
doi = {10.1038/nature09935},
eprint = {1103.5805},
journal = {\nat},
month = {mar},
pages = {608-611},
primaryclass = {astro-ph.SR},
title = {{Gravity modes as a way to distinguish between hydrogen- and helium-burning red giant stars}},
volume = {471},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature09935},
}
@inproceedings{borucki09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009IAUS..253..289B},
author = {{Borucki}, W. and {Koch}, D. and {Batalha}, N. and {Caldwell}, D. and {Christensen-Dalsgaard}, J. and {Cochran}, W.~D. and {Dunham}, E. and {Gautier}, T.~N. and {Geary}, J. and {Gilliland}, R. and {Jenkins}, J. and {Kjeldsen}, H. and {Lissauer}, J.~J. and {Rowe}, J.},
booktitle = {Proc. IAU Symp. 253},
doi = {10.1017/S1743921308026513},
month = {feb},
pages = {289-299},
title = {{KEPLER: Search for Earth-Size Planets in the Habitable Zone}},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1017/S1743921308026513},
}
@article{brown91,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1991ApJ...368..599B},
author = {{Brown}, T.~M. and {Gilliland}, R.~L. and {Noyes}, R.~W. and {Ramsey}, L.~W.},
doi = {10.1086/169725},
journal = {\apj},
keywords = {F STARS, LATE STARS, STELLAR OSCILLATIONS, SUBGIANT STARS, CHARGE COUPLED DEVICES, DOPPLER EFFECT, POWER SPECTRA, STELLAR LUMINOSITY, STELLAR TEMPERATURE},
month = {feb},
pages = {599-609},
title = {{Detection of possible p-mode oscillations on Procyon}},
volume = {368},
year = {1991},
bdsk-url-1 = {http://dx.doi.org/10.1086/169725},
}
@article{christen04,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2004SoPh..220..137C},
author = {{Christensen-Dalsgaard}, J.},
doi = {10.1023/B:SOLA.0000031392.43227.7d},
journal = {\solphys},
month = {apr},
pages = {137-168},
title = {{Physics of solar-like oscillations}},
volume = {220},
year = {2004},
bdsk-url-1 = {http://dx.doi.org/10.1023/B:SOLA.0000031392.43227.7d},
}
@article{christen11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1106.5946C},
archiveprefix = {arXiv},
author = {{Christensen-Dalsgaard}, J.},
eprint = {1106.5946},
journal = {\arXiv:1106.5946},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {jun},
primaryclass = {astro-ph.SR},
title = {{Asteroseismology of red giants}},
year = {2011},
}
@article{deheuvels11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1109.1191D},
archiveprefix = {arXiv},
author = {{Deheuvels}, S. and {Michel}, E.},
eprint = {1109.1191},
journal = {ArXiv e-prints},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {sep},
primaryclass = {astro-ph.SR},
title = {{Constraints on the structure of the core of subgiants via mixed modes: the case of HD49385}},
year = {2011},
}
@article{denissenkov07,
author = {{Denissenkov}, P.~A. and {Pinsonneault}, M.},
journal = {\apj},
month = {feb},
pages = {1157-1165},
title = {{A Revised Prescription for the Tayler-Spruit Dynamo: Magnetic Angular Momentum Transport in Stars}},
volume = {655},
year = {2007},
}
@article{deridder09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009Natur.459..398D},
author = {{De Ridder}, J. and {Barban}, C. and {Baudin}, F. and {Carrier}, F. and {Hatzes}, A.~P. and {Hekker}, S. and {Kallinger}, T. and {Weiss}, W.~W. and {Baglin}, A. and {Auvergne}, M. and {Samadi}, R. and {Barge}, P. and {Deleuil}, M.},
doi = {10.1038/nature08022},
journal = {\nat},
month = {may},
pages = {398-400},
title = {{Non-radial oscillation modes with long lifetimes in giant stars}},
volume = {459},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature08022},
}
@article{dimauro11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011MNRAS.415.3783D},
archiveprefix = {arXiv},
author = {{di Mauro}, M.~P. and {Cardini}, D. and {Catanzaro}, G. and {Ventura}, R. and {Barban}, C. and {Bedding}, T.~R. and {Christensen-Dalsgaard}, J. and {De Ridder}, J. and {Hekker}, S. and {Huber}, D. and {Kallinger}, T. and {Miglio}, A. and {Montalban}, J. and {Mosser}, B. and {Stello}, D. and {Uytterhoeven}, K. and {Kinemuchi}, K. and {Kjeldsen}, H. and {Mullally}, F. and {Still}, M.},
doi = {10.1111/j.1365-2966.2011.18996.x},
eprint = {1105.1076},
journal = {\mnras},
keywords = {stars: AGB and post-AGB, stars: evolution, stars: fundamental parameters, stars: individual: KIC 4351319, stars: oscillations, stars: solar-type},
month = {aug},
pages = {3783-3797},
primaryclass = {astro-ph.SR},
title = {{Solar-like oscillations from the depths of the red-giant star KIC 4351319 observed with Kepler}},
volume = {415},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2011.18996.x},
}
@article{dominguez99,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1999ApJ...524..226D},
author = {{Dominguez}, I. and {Chieffi}, A. and {Limongi}, M. and {Straniero}, O.},
doi = {10.1086/307787},
eprint = {arXiv:astro-ph/9906030},
journal = {\apj},
keywords = {GALAXY: OPEN CLUSTERS AND ASSOCIATIONS: GENERAL, STARS: EVOLUTION, STARS: INTERIORS},
month = {oct},
pages = {226-241},
title = {{Intermediate-Mass Stars: Updated Models}},
volume = {524},
year = {1999},
bdsk-url-1 = {http://dx.doi.org/10.1086/307787},
}
@article{dupret09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009A%26A...506...57D},
archiveprefix = {arXiv},
author = {{Dupret}, M.-A. and {Belkacem}, K. and {Samadi}, R. and {Montalban}, J. and {Moreira}, O. and {Miglio}, A. and {Godart}, M. and {Ventura}, P. and {Ludwig}, H.-G. and {Grigahc{\`e}ne}, A. and {Goupil}, M.-J. and {Noels}, A. and {Caffau}, E.},
doi = {10.1051/0004-6361/200911713},
eprint = {0906.3951},
journal = {\aap},
keywords = {stars: oscillations, stars: interiors, convection},
month = {oct},
pages = {57-67},
primaryclass = {astro-ph.SR},
title = {{Theoretical amplitudes and lifetimes of non-radial solar-like oscillations in red giants}},
volume = {506},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/200911713},
}
@article{dziembowski01,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2001MNRAS.328..601D},
author = {{Dziembowski}, W.~A. and {Gough}, D.~O. and {Houdek}, G. and {Sienkiewicz}, R.},
doi = {10.1046/j.1365-8711.2001.04894.x},
eprint = {arXiv:astro-ph/0108337},
journal = {\mnras},
keywords = {CONVECTION, STARS: INDIVIDUAL: {$\alpha$}UMA, STARS: OSCILLATIONS},
month = {dec},
pages = {601-610},
title = {{Oscillations of {$\alpha$} UMa and other red giants}},
volume = {328},
year = {2001},
bdsk-url-1 = {http://dx.doi.org/10.1046/j.1365-8711.2001.04894.x},
}
@article{ferguson05,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2005ApJ...623..585F},
author = {{Ferguson}, J.~W. and {Alexander}, D.~R. and {Allard}, F. and {Barman}, T. and {Bodnarik}, J.~G. and {Hauschildt}, P.~H. and {Heffner-Wong}, A. and {Tamanai}, A.},
doi = {10.1086/428642},
eprint = {arXiv:astro-ph/0502045},
journal = {\apj},
keywords = {Atomic Data, Equation of State, Methods: Numerical, Molecular Data},
month = {apr},
pages = {585-596},
title = {{Low-Temperature Opacities}},
volume = {623},
year = {2005},
bdsk-url-1 = {http://dx.doi.org/10.1086/428642},
}
@article{grevesse98,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1998SSRv...85..161G},
author = {{Grevesse}, N. and {Sauval}, A.~J.},
doi = {10.1023/A:1005161325181},
journal = {\ssr},
keywords = {Sun: abundances, Meteorites: abundances, Solar spectroscopy},
month = {may},
pages = {161-174},
title = {{Standard Solar Composition}},
volume = {85},
year = {1998},
bdsk-url-1 = {http://dx.doi.org/10.1023/A:1005161325181},
}
@article{heger05,
author = {{Heger}, A. and {Woosley}, S.~E. and {Spruit}, H.~C.},
journal = {\apj},
month = {jun},
pages = {350-363},
title = {{Presupernova Evolution of Differentially Rotating Massive Stars Including Magnetic Fields}},
volume = {626},
year = {2005},
}
@article{hekker09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009A%26A...506..465H},
archiveprefix = {arXiv},
author = {{Hekker}, S. and {Kallinger}, T. and {Baudin}, F. and {De Ridder}, J. and {Barban}, C. and {Carrier}, F. and {Hatzes}, A.~P. and {Weiss}, W.~W. and {Baglin}, A.},
doi = {10.1051/0004-6361/200911858},
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month = {oct},
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title = {{Characteristics of solar-like oscillations in red giants observed in the CoRoT exoplanet field}},
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}
@article{hekker11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011MNRAS.414.2594H},
archiveprefix = {arXiv},
author = {{Hekker}, S. and {Gilliland}, R.~L. and {Elsworth}, Y. and {Chaplin}, W.~J. and {De Ridder}, J. and {Stello}, D. and {Kallinger}, T. and {Ibrahim}, K.~A. and {Klaus}, T.~C. and {Li}, J.},
doi = {10.1111/j.1365-2966.2011.18574.x},
eprint = {1103.0141},
journal = {\mnras},
keywords = {methods: observational, techniques: photometric, stars: late type, stars: oscillations},
month = {jul},
pages = {2594-2601},
primaryclass = {astro-ph.SR},
title = {{Characterization of red giant stars in the public Kepler data}},
volume = {414},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2011.18574.x},
}
@article{huber11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1109.3460H},
archiveprefix = {arXiv},
author = {{Huber}, D. and {Bedding}, T.~R. and {Stello}, D. and {Hekker}, S. and {Mathur}, S. and {Mosser}, B. and {Verner}, G.~A. and {Bonanno}, A. and {Buzasi}, D.~L. and {Campante}, T.~L. and {Elsworth}, Y.~P. and {Hale}, S.~J. and {Kallinger}, T. and {Silva Aguirre}, V. and {Chaplin}, W.~J. and {De Ridder}, J. and {Garcia}, R.~A. and {Appourchaux}, T. and {Frandsen}, S. and {Houdek}, G. and {Molenda-Zakowicz}, J. and {Monteiro}, M.~J.~P.~F.~G. and {Christensen-Dalsgaard}, J. and {Gilliland}, R.~L. and {Kawaler}, S.~D. and {Kjeldsen}, H. and {Broomhall}, A.~M. and {Corsaro}, E. and {Salabert}, D. and {Sanderfer}, D.~T. and {Seader}, S.~E. and {Smith}, J.~C.},
eprint = {1109.3460},
journal = {ArXiv e-prints},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {sep},
primaryclass = {astro-ph.SR},
title = {{Testing Scaling Relations for Solar-Like Oscillations from the Main Sequence to Red Giants using Kepler Data}},
year = {2011},
}
@article{huber10,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...723.1607H},
archiveprefix = {arXiv},
author = {{Huber}, D. and {Bedding}, T.~R. and {Stello}, D. and {Mosser}, B. and {Mathur}, S. and {Kallinger}, T. and {Hekker}, S. and {Elsworth}, Y.~P. and {Buzasi}, D.~L. and {De Ridder}, J. and {Gilliland}, R.~L. and {Kjeldsen}, H. and {Chaplin}, W.~J. and {Garc{\'{\i}}a}, R.~A. and {Hale}, S.~J. and {Preston}, H.~L. and {White}, T.~R. and {Borucki}, W.~J. and {Christensen-Dalsgaard}, J. and {Clarke}, B.~D. and {Jenkins}, J.~M. and {Koch}, D.},
doi = {10.1088/0004-637X/723/2/1607},
eprint = {1010.4566},
journal = {\apj},
keywords = {stars: late-type, stars: oscillations},
month = {nov},
pages = {1607-1617},
primaryclass = {astro-ph.SR},
title = {{Asteroseismology of Red Giants from the First Four Months of Kepler Data: Global Oscillation Parameters for 800 Stars}},
volume = {723},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/723/2/1607},
}
@article{ibenrenzini84,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1984PhR...105..329I},
author = {{Iben}, I. and {Renzini}, A.},
doi = {10.1016/0370-1573(84)90142-X},
journal = {\physrep},
month = {mar},
pages = {329-406},
title = {{Single star evolution I. Massive stars and early evolution of low and intermediate mass stars}},
volume = {105},
year = {1984},
bdsk-url-1 = {http://dx.doi.org/10.1016/0370-1573(84)90142-X},
}
@article{iglesias96,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1996ApJ...464..943I},
author = {{Iglesias}, C.~A. and {Rogers}, F.~J.},
doi = {10.1086/177381},
journal = {\apj},
keywords = {ATOMIC DATA, ATOMIC PROCESSES, STARS: INTERIORS},
month = {jun},
pages = {943-953},
title = {{Updated Opal Opacities}},
volume = {464},
year = {1996},
bdsk-url-1 = {http://dx.doi.org/10.1086/177381},
}
@article{jiang11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1109.0962J},
archiveprefix = {arXiv},
author = {{Jiang}, C. and {Jiang}, B. and {Christensen-Dalsgaard}, J. and {Bedding}, T.~R. and {Stello}, D. and {Huber}, D. and {Fandsen}, S. and {Kjeldsen}, H. and {Karoff}, C. and {Mosser}, B. and {Demarque}, P. and {Fanelli}, M.~N. and {Kinemuchi}, K. and {Mullally}, F.},
eprint = {1109.0962},
journal = {ArXiv e-prints},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {sep},
primaryclass = {astro-ph.SR},
title = {{Modelling Kepler Observations of Solar-like Oscillations in the Red-giant Star HD 186355}},
year = {2011},
}
@article{kjeldsen95,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1995A%26A...293...87K},
author = {{Kjeldsen}, H. and {Bedding}, T.~R.},
eprint = {arXiv:astro-ph/9403015},
journal = {\aap},
keywords = {SUN: OSCILLATIONS, STARS: INDIVIDUAL: $\{$ALPHA$\}$ CEN, STARS: INDIVIDUAL: PROCYON, STARS: OSCILLATIONS, CEPHEIDS, $\{$DELTA$\}$ SCT},
month = {jan},
pages = {87-106},
title = {{Amplitudes of stellar oscillations: the implications for asteroseismology.}},
volume = {293},
year = {1995},
}
@article{maeder05,
author = {{Maeder}, A. and {Meynet}, G.},
journal = {\aap},
month = {sep},
pages = {1041-1049},
title = {{Stellar evolution with rotation and magnetic fields. III. The interplay of circulation and dynamo}},
volume = {440},
year = {2005},
}
@article{maeder04,
author = {{Maeder}, A. and {Meynet}, G.},
journal = {\aap},
month = {jul},
pages = {225-237},
title = {{Stellar evolution with rotation and magnetic fields. II. General equations for the transport by Tayler-Spruit dynamo}},
volume = {422},
year = {2004},
}
@article{maeder03,
author = {{Maeder}, A. and {Meynet}, G.},
journal = {\aap},
month = {dec},
pages = {543-552},
title = {{Stellar evolution with rotation and magnetic fields. I. The relative importance of rotational and magnetic effects}},
volume = {411},
year = {2003},
}
@article{maeder98,
author = {{Maeder}, A. and {Zahn}, J.-P.},
journal = {\aap},
month = {jun},
pages = {1000-1006},
title = {{Stellar evolution with rotation. III. Meridional circulation with $\mu$-gradients and non-stationarity}},
volume = {334},
year = {1998},
}
@article{meynet97,
author = {{Meynet}, G. and {Maeder}, A.},
journal = {\aap},
month = {may},
pages = {465-476},
title = {{Stellar evolution with rotation. I. The computational method and the inhibiting effect of the $\mu$-gradient}},
volume = {321},
year = {1997},
}
@article{miglio09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009A%26A...503L..21M},
archiveprefix = {arXiv},
author = {{Miglio}, A. and {Montalb{\'a}n}, J. and {Baudin}, F. and {Eggenberger}, P. and {Noels}, A. and {Hekker}, S. and {De Ridder}, J. and {Weiss}, W. and {Baglin}, A.},
doi = {10.1051/0004-6361/200912822},
eprint = {0908.0210},
journal = {\aap},
keywords = {stars: fundamental parameters, stars: horizontal-branch, stars: mass-loss, stars: oscillations, galaxy: disk, galaxy: stellar content},
month = {sep},
pages = {L21-L24},
primaryclass = {astro-ph.SR},
title = {{Probing populations of red giants in the galactic disk with CoRoT}},
volume = {503},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/200912822},
}
@article{miglio11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1108.4555M},
archiveprefix = {arXiv},
author = {{Miglio}, A.},
eprint = {1108.4555},
journal = {ArXiv e-prints},
keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Galaxy Astrophysics},
month = {aug},
primaryclass = {astro-ph.SR},
title = {{Asteroseismology of red giants as a tool for studying stellar populations: first steps}},
year = {2011},
}
@article{mocak08,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008A%26A...490..265M},
archiveprefix = {arXiv},
author = {{Moc{\'a}k}, M. and {M{\"u}ller}, E. and {Weiss}, A. and {Kifonidis}, K.},
doi = {10.1051/0004-6361:200810169},
eprint = {0805.1355},
journal = {\aap},
keywords = {stars: evolution, hydrodynamics, convection, stars: interiors},
month = {oct},
pages = {265-277},
title = {{The core helium flash revisited. I. One and two-dimensional hydrodynamic simulations}},
volume = {490},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:200810169},
}
@article{mocak09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009A%26A...501..659M},
archiveprefix = {arXiv},
author = {{Moc{\'a}k}, M. and {M{\"u}ller}, E. and {Weiss}, A. and {Kifonidis}, K.},
doi = {10.1051/0004-6361/200811414},
eprint = {0811.4083},
journal = {\aap},
keywords = {stars: evolution, hydrodynamics, convection, stars: interiors},
month = {jul},
pages = {659-677},
title = {{The core helium flash revisited. II. Two and three-dimensional hydrodynamic simulations}},
volume = {501},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/200811414},
}
@article{montalban10,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...721L.182M},
archiveprefix = {arXiv},
author = {{Montalb{\'a}n}, J. and {Miglio}, A. and {Noels}, A. and {Scuflaire}, R. and {Ventura}, P.},
doi = {10.1088/2041-8205/721/2/L182},
eprint = {1009.1754},
journal = {\apjl},
keywords = {stars: evolution, stars: interiors, stars: late-type, stars: oscillations},
month = {oct},
pages = {L182-L188},
primaryclass = {astro-ph.SR},
title = {{Seismic Diagnostics of Red Giants: First Comparison with Stellar Models}},
volume = {721},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/721/2/L182},
}
@article{mosser10,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...517A..22M},
archiveprefix = {arXiv},
author = {{Mosser}, B. and {Belkacem}, K. and {Goupil}, M.-J. and {Miglio}, A. and {Morel}, T. and {Barban}, C. and {Baudin}, F. and {Hekker}, S. and {Samadi}, R. and {De Ridder}, J. and {Weiss}, W. and {Auvergne}, M. and {Baglin}, A.},
doi = {10.1051/0004-6361/201014036},
eprint = {1004.0449},
journal = {\aap},
keywords = {stars: fundamental parameters, stars: interiors, stars: evolution, stars: oscillations, stars: abundances},
month = {jul},
pages = {A22, 11pp},
primaryclass = {astro-ph.SR},
title = {{Red-giant seismic properties analyzed with CoRoT}},
volume = {517},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201014036},
}
@article{mosser11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011A%26A...525L...9M},
archiveprefix = {arXiv},
author = {{Mosser}, B. and {Belkacem}, K. and {Goupil}, M.~J. and {Michel}, E. and {Elsworth}, Y. and {Barban}, C. and {Kallinger}, T. and {Hekker}, S. and {De Ridder}, J. and {Samadi}, R. and {Baudin}, F. and {Pinheiro}, F.~J.~G. and {Auvergne}, M. and {Baglin}, A. and {Catala}, C.},
doi = {10.1051/0004-6361/201015440},
eprint = {1011.1928},
journal = {\aap},
keywords = {stars: oscillations, stars: interiors, methods: data analysis, methods: analytical},
month = {jan},
pages = {L9, 4pp},
primaryclass = {astro-ph.SR},
title = {{The universal red-giant oscillation pattern. An automated determination with CoRoT data}},
volume = {525},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201015440},
}
@article{mosser11mixed,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011A%26A...532A..86M},
archiveprefix = {arXiv},
author = {{Mosser}, B. and {Barban}, C. and {Montalb{\'a}n}, J. and {Beck}, P.~G. and {Miglio}, A. and {Belkacem}, K. and {Goupil}, M.~J. and {Hekker}, S. and {De Ridder}, J. and {Dupret}, M.~A. and {Elsworth}, Y. and {Noels}, A. and {Baudin}, F. and {Michel}, E. and {Samadi}, R. and {Auvergne}, M. and {Baglin}, A. and {Catala}, C.},
doi = {10.1051/0004-6361/201116825},
eprint = {1105.6113},
journal = {\aap},
keywords = {stars: oscillations, stars: interiors, stars: mass-loss, methods: data analysis},
month = {aug},
pages = {A86, 8pp},
primaryclass = {astro-ph.SR},
title = {{Mixed modes in red-giant stars observed with CoRoT}},
volume = {532},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201116825},
}
@article{osaki75,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1975PASJ...27..237O},
author = {{Osaki}, J.},
journal = {\pasj},
keywords = {ASTRONOMICAL MODELS, EIGENVECTORS, MAIN SEQUENCE STARS, STELLAR MASS, VARIABLE STARS, DYNAMIC STABILITY, GRAVITATIONAL WAVES, PULSED RADIATION, STELLAR EVOLUTION, VIBRATION MODE},
pages = {237-258},
title = {{Nonradial oscillations of a 10 solar mass star in the main-sequence stage}},
volume = {27},
year = {1975},
}
@article{paxton11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJS..192....3P},
archiveprefix = {arXiv},
author = {{Paxton}, B. and {Bildsten}, L. and {Dotter}, A. and {Herwig}, F. and {Lesaffre}, P. and {Timmes}, F.},
doi = {10.1088/0067-0049/192/1/3},
eprint = {1009.1622},
journal = {\apjs},
keywords = {methods: numerical, stars: evolution, stars: general},
month = {jan},
pages = {3, 35pp},
primaryclass = {astro-ph.SR},
title = {{Modules for Experiments in Stellar Astrophysics (MESA)}},
volume = {192},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/0067-0049/192/1/3},
}
@article{rogers02,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2002ApJ...576.1064R},
author = {{Rogers}, F.~J. and {Nayfonov}, A.},
doi = {10.1086/341894},
journal = {\apj},
keywords = {Atomic Processes, Equation of State, Sun: Oscillations},
month = {sep},
pages = {1064-1074},
title = {{Updated and Expanded OPAL Equation-of-State Tables: Implications for Helioseismology}},
volume = {576},
year = {2002},
bdsk-url-1 = {http://dx.doi.org/10.1086/341894},
}
@article{salaris02,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2002PASP..114..375S},
author = {{Salaris}, M. and {Cassisi}, S. and {Weiss}, A.},
doi = {10.1086/342498},
eprint = {arXiv:astro-ph/0201387},
journal = {\pasp},
keywords = {Galaxy: Globular Clusters: General, Stars: Hertzsprung-Russell Diagram, nuclear reactions, nucleosynthesis, abundances, Stars: Atmospheres, Stars: Evolution, Stars: Interiors},
month = {apr},
pages = {375-402},
title = {{Red Giant Branch Stars: The Theoretical Framework}},
volume = {114},
year = {2002},
bdsk-url-1 = {http://dx.doi.org/10.1086/342498},
}
@article{scuflaire74,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1974A%26A....36..107S},
author = {{Scuflaire}, R.},
journal = {\aap},
month = {nov},
pages = {107-111},
title = {{The Non Radial Oscillations of Condensed Polytropes}},
volume = {36},
year = {1974},
}
@article{serenelli05,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2005A%26A...442.1041S},
author = {{Serenelli}, A. and {Weiss}, A.},
doi = {10.1051/0004-6361:20053390},
eprint = {arXiv:astro-ph/0507430},
journal = {\aap},
keywords = {stars: evolution, stars: horizontal-branch, methods: numerical},
month = {nov},
pages = {1041-1048},
title = {{On constructing horizontal branch models}},
volume = {442},
year = {2005},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20053390},
}
@article{serenellif05,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2005ApJ...632L..33S},
author = {{Serenelli}, A.~M. and {Fukugita}, M.},
doi = {10.1086/497535},
eprint = {arXiv:astro-ph/0505333},
journal = {\apjl},
keywords = {Neutrinos, Stars: Evolution},
month = {oct},
pages = {L33-L36},
title = {{Burst Neutrinos from the Nitrogen Flash}},
volume = {632},
year = {2005},
bdsk-url-1 = {http://dx.doi.org/10.1086/497535},
}
@article{shen09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...699.1365S},
archiveprefix = {arXiv},
author = {{Shen}, K.~J. and {Bildsten}, L.},
doi = {10.1088/0004-637X/699/2/1365},
eprint = {0903.0654},
journal = {\apj},
keywords = {binaries: close, novae, cataclysmic variables, supernovae: general, white dwarfs},
month = {jul},
pages = {1365-1373},
primaryclass = {astro-ph.HE},
title = {{Unstable Helium Shell Burning on Accreting White Dwarfs}},
volume = {699},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/699/2/1365},
}
@article{spruit99,
author = {{Spruit}, H.~C.},
journal = {\aap},
month = {sep},
pages = {189-202},
title = {{Differential rotation and magnetic fields in stellar interiors}},
volume = {349},
year = {1999},
}
@article{silva08,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008A%26A...489.1201S},
archiveprefix = {arXiv},
author = {{Silva Aguirre}, V. and {Catelan}, M. and {Weiss}, A. and {Valcarce}, A.~A.~R.},
doi = {10.1051/0004-6361:200810047},
eprint = {0807.3017},
journal = {\aap},
keywords = {stars: evolution, stars: Hertzsprung-Russell (HR) and C-M diagrams, stars: horizontal-branch, stars: oscillations, stars: variables: RR Lyr, Galaxy: globular clusters: individual: NGC 5272},
month = {oct},
pages = {1201-1208},
title = {{Stellar evolution and variability in the pre-ZAHB phase}},
volume = {489},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:200810047},
}
@article{stello09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009MNRAS.400L..80S},
archiveprefix = {arXiv},
author = {{Stello}, D. and {Chaplin}, W.~J. and {Basu}, S. and {Elsworth}, Y. and {Bedding}, T.~R.},
doi = {10.1111/j.1745-3933.2009.00767.x},
eprint = {0909.5193},
journal = {\mnras},
keywords = {stars: fundamental parameters , stars: interiors , stars: oscillations},
month = {nov},
pages = {L80-L84},
primaryclass = {astro-ph.SR},
title = {{The relation between {$\Delta$}{$\nu$} and {$\nu$}$_{max}$ for solar-like oscillations}},
volume = {400},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1745-3933.2009.00767.x},
}
@article{thomas67,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1967ZA.....67..420T},
author = {{Thomas}, H.-C.},
journal = {\zap},
pages = {420-455},
title = {{Sternentwicklung VIII. Der Helium-Flash bei einem Stern von 1. 3 Sonnenmassen}},
volume = {67},
year = {1967},
}
@article{timmes00,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000ApJS..126..501T},
author = {{Timmes}, F.~X. and {Swesty}, F.~D.},
journal = {\apjs},
keywords = {EQUATION OF STATE, HYDRODYNAMICS, METHODS: NUMERICAL, STARS: GENERAL},
month = {feb},
pages = {501-516},
title = {{The Accuracy, Consistency, and Speed of an Electron-Positron Equation of State Based on Table Interpolation of the Helmholtz Free Energy}},
volume = {126},
year = {2000},
}
@book{unno89,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1989nos..book.....U},
author = {{Unno}, W. and {Osaki}, Y. and {Ando}, H. and {Saio}, H. and {Shibahashi}, H.},
booktitle = {Nonradial oscillations of stars, Tokyo: University of Tokyo Press, 1989, 2nd ed.},
editor = {{Unno, W., Osaki, Y., Ando, H., Saio, H., \& Shibahashi, H.}},
title = {{Nonradial oscillations of stars}},
year = {1989},
}
@article{white11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011arXiv1109.3455W},
archiveprefix = {arXiv},
author = {{White}, T.~R. and {Bedding}, T.~R. and {Stello}, D. and {Christensen-Dalsgaard}, J. and {Huber}, D. and {Kjeldsen}, H.},
eprint = {1109.3455},
journal = {ArXiv e-prints},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {sep},
primaryclass = {astro-ph.SR},
title = {{Calculating asteroseismic diagrams for solar-like oscillations}},
year = {2011},
}
@article{zahn07,
author = {{Zahn}, J.-P. and {Brun}, A.~S. and {Mathis}, S.},
journal = {\aap},
month = {oct},
pages = {145-154},
title = {{On magnetic instabilities and dynamo action in stellar radiation zones}},
volume = {474},
year = {2007},
}
@article{Paxton:2013,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2013arXiv1301.0319P},
archiveprefix = {arXiv},
author = {{Paxton}, B. and {Cantiello}, M. and {Arras}, P. and {Bildsten}, L. and {Brown}, E.~F. and {Dotter}, A. and {Mankovich}, C. and {Montgomery}, M.~H. and {Stello}, D. and {Timmes}, F.~X. and {Townsend}, R.},
eprint = {1301.0319},
journal = {\arXiv:1301.0319},
keywords = {Astrophysics - Solar and Stellar Astrophysics, Astrophysics - Instrumentation and Methods for Astrophysics},
month = {jan},
primaryclass = {astro-ph.SR},
title = {{Modules for Experiments in Stellar Astrophysics (MESA): Giant Planets, Oscillations, Rotation, and Massive Stars}},
year = {2013},
}
@article{Joss:1973,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1973ApJ...181..429J},
author = {{Joss}, P.~C. and {Salpeter}, E.~E. and {Ostriker}, J.~P.},
doi = {10.1086/152060},
journal = {\apj},
month = {apr},
pages = {429-438},
title = {{On the ``critical Luminosity'' in Stellar Interiors and Stellar Surface Boundary Conditions}},
volume = {181},
year = {1973},
bdsk-url-1 = {http://dx.doi.org/10.1086/152060},
}
@article{2013ApJ...762....8D,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...762....8D},
archiveprefix = {arXiv},
author = {{Denissenkov}, P.~A. and {Herwig}, F. and {Bildsten}, L. and {Paxton}, B.},
doi = {10.1088/0004-637X/762/1/8},
eid = {8},
eprint = {1210.5209},
journal = {\apj},
keywords = {methods: numerical, novae, cataclysmic variables, stars: abundances, stars: evolution, stars: interiors},
month = {jan},
pages = {8, 10pp},
primaryclass = {astro-ph.SR},
title = {{MESA Models of Classical Nova Outbursts: The Multicycle Evolution and Effects of Convective Boundary Mixing}},
volume = {762},
year = {2013},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/762/1/8},
}
@article{2012ApJ...761..182M,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...761..182M},
archiveprefix = {arXiv},
author = {{Moore}, K. and {Bildsten}, L.},
doi = {10.1088/0004-637X/761/2/182},
eid = {182},
eprint = {1210.7546},
journal = {\apj},
keywords = {binaries: symbiotic, circumstellar matter, novae, cataclysmic variables, shock waves, supernovae: general},
month = {dec},
pages = {182, 7pp},
primaryclass = {astro-ph.SR},
title = {{Circumstellar Shell Formation in Symbiotic Recurrent Novae}},
volume = {761},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/761/2/182},
}
@article{2012ApJ...758...64K,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...758...64K},
archiveprefix = {arXiv},
author = {{Kaplan}, D.~L. and {Bildsten}, L. and {Steinfadt}, J.~D.~R.},
doi = {10.1088/0004-637X/758/1/64},
eid = {64},
eprint = {1208.6320},
journal = {\apj},
keywords = {nuclear reactions, nucleosynthesis, abundances, supernovae: individual: Type Ia, white dwarfs},
month = {oct},
pages = {64, 11pp},
primaryclass = {astro-ph.SR},
title = {{Orbital Evolution of Compact White Dwarf Binaries}},
volume = {758},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/758/1/64},
}
@article{2012Sci...337..942D,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012Sci...337..942D},
archiveprefix = {arXiv},
author = {{Dilday}, B. and {Howell}, D.~A. and {Cenko}, S.~B. and {Silverman}, J.~M. and {Nugent}, P.~E. and {Sullivan}, M. and {Ben-Ami}, S. and {Bildsten}, L. and {Bolte}, M. and {Endl}, M. and {Filippenko}, A.~V. and {Gnat}, O. and {Horesh}, A. and {Hsiao}, E. and {Kasliwal}, M.~M. and {Kirkman}, D. and {Maguire}, K. and {Marcy}, G.~W. and {Moore}, K. and {Pan}, Y. and {Parrent}, J.~T. and {Podsiadlowski}, P. and {Quimby}, R.~M. and {Sternberg}, A. and {Suzuki}, N. and {Tytler}, D.~R. and {Xu}, D. and {Bloom}, J.~S. and {Gal-Yam}, A. and {Hook}, I.~M. and {Kulkarni}, S.~R. and {Law}, N.~M. and {Ofek}, E.~O. and {Polishook}, D. and {Poznanski}, D.},
doi = {10.1126/science.1219164},
eprint = {1207.1306},
journal = {\sci},
month = {aug},
pages = {942-945},
primaryclass = {astro-ph.CO},
title = {{PTF 11kx: A Type Ia Supernova with a Symbiotic Nova Progenitor}},
volume = {337},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1126/science.1219164},
}
@article{2012PASP..124..854O,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012PASP..124..854O},
archiveprefix = {arXiv},
author = {{Ofek}, E.~O. and {Laher}, R. and {Surace}, J. and {Levitan}, D. and {Sesar}, B. and {Horesh}, A. and {Law}, N. and {van Eyken}, J.~C. and {Kulkarni}, S.~R. and {Prince}, T.~A. and {Nugent}, P. and {Sullivan}, M. and {Yaron}, O. and {Pickles}, A. and {Ag{\"u}eros}, M. and {Arcavi}, I. and {Bildsten}, L. and {Bloom}, J. and {Cenko}, S.~B. and {Gal-Yam}, A. and {Grillmair}, C. and {Helou}, G. and {Kasliwal}, M.~M. and {Poznanski}, D. and {Quimby}, R.},
doi = {10.1086/666978},
eprint = {1206.1064},
journal = {\pasp},
keywords = {Astronomical Techniques},
month = {aug},
pages = {854-860},
primaryclass = {astro-ph.IM},
title = {{The Palomar Transient Factory photometric catalog 1.0}},
volume = {124},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1086/666978},
}
@article{2012ApJ...755..161K,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...755..161K},
archiveprefix = {arXiv},
author = {{Kasliwal}, M.~M. and {Kulkarni}, S.~R. and {Gal-Yam}, A. and {Nugent}, P.~E. and {Sullivan}, M. and {Bildsten}, L. and {Yaron}, O. and {Perets}, H.~B. and {Arcavi}, I. and {Ben-Ami}, S. and {Bhalerao}, V.~B. and {Bloom}, J.~S. and {Cenko}, S.~B. and {Filippenko}, A.~V. and {Frail}, D.~A. and {Ganeshalingam}, M. and {Horesh}, A. and {Howell}, D.~A. and {Law}, N.~M. and {Leonard}, D.~C. and {Li}, W. and {Ofek}, E.~O. and {Polishook}, D. and {Poznanski}, D. and {Quimby}, R.~M. and {Silverman}, J.~M. and {Sternberg}, A. and {Xu}, D.},
doi = {10.1088/0004-637X/755/2/161},
eid = {161},
eprint = {1111.6109},
journal = {\apj},
keywords = {galaxies: clusters: general, Galaxy: halo, novae, cataclysmic variables, supernovae: individual: SN2005E SN2007ke PTF09dav PTF10iuv PTF11bij, surveys, white dwarfs},
month = {aug},
pages = {161, 14pp},
primaryclass = {astro-ph.HE},
title = {{Calcium-rich Gap Transients in the Remote Outskirts of Galaxies}},
volume = {755},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/755/2/161},
}
@article{2012ApJ...755....4T,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...755....4T},
archiveprefix = {arXiv},
author = {{Townsley}, D.~M. and {Moore}, K. and {Bildsten}, L.},
doi = {10.1088/0004-637X/755/1/4},
eid = {4},
eprint = {1205.6517},
journal = {\apj},
keywords = {hydrodynamics, nuclear reactions, nucleosynthesis, abundances, white dwarfs},
month = {aug},
pages = {4, 6pp},
primaryclass = {astro-ph.SR},
title = {{Laterally Propagating Detonations in Thin Helium Layers on Accreting White Dwarfs}},
volume = {755},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/755/1/4},
}
@article{2012ApJ...752L..26P,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...752L..26P},
archiveprefix = {arXiv},
author = {{Parrent}, J.~T. and {Howell}, D.~A. and {Friesen}, B. and {Thomas}, R.~C. and {Fesen}, R.~A. and {Milisavljevic}, D. and {Bianco}, F.~B. and {Dilday}, B. and {Nugent}, P. and {Baron}, E. and {Arcavi}, I. and {Ben-Ami}, S. and {Bersier}, D. and {Bildsten}, L. and {Bloom}, J. and {Cao}, Y. and {Cenko}, S.~B. and {Filippenko}, A.~V. and {Gal-Yam}, A. and {Kasliwal}, M.~M. and {Konidaris}, N. and {Kulkarni}, S.~R. and {Law}, N.~M. and {Levitan}, D. and {Maguire}, K. and {Mazzali}, P.~A. and {Ofek}, E.~O. and {Pan}, Y. and {Polishook}, D. and {Poznanski}, D. and {Quimby}, R.~M. and {Silverman}, J.~M. and {Sternberg}, A. and {Sullivan}, M. and {Walker}, E.~S. and {Xu}, D. and {Buton}, C. and {Pereira}, R.},
doi = {10.1088/2041-8205/752/2/L26},
eid = {L26, 7pp},
eprint = {1205.6011},
journal = {\apjl},
keywords = {supernovae: general, supernovae: individual: SN 2011fe},
month = {jun},
pages = {L26},
primaryclass = {astro-ph.CO},
title = {{Analysis of the Early-time Optical Spectra of SN 2011fe in M101}},
volume = {752},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/752/2/L26},
}
@article{2012MNRAS.420.2684C,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012MNRAS.420.2684C},
archiveprefix = {arXiv},
author = {{Cenko}, S.~B. and {Bloom}, J.~S. and {Kulkarni}, S.~R. and {Strubbe}, L.~E. and {Miller}, A.~A. and {Butler}, N.~R. and {Quimby}, R.~M. and {Gal-Yam}, A. and {Ofek}, E.~O. and {Quataert}, E. and {Bildsten}, L. and {Poznanski}, D. and {Perley}, D.~A. and {Morgan}, A.~N. and {Filippenko}, A.~V. and {Frail}, D.~A. and {Arcavi}, I. and {Ben-Ami}, S. and {Cucchiara}, A. and {Fassnacht}, C.~D. and {Green}, Y. and {Hook}, I.~M. and {Howell}, D.~A. and {Lagattuta}, D.~J. and {Law}, N.~M. and {Kasliwal}, M.~M. and {Nugent}, P.~E. and {Silverman}, J.~M. and {Sullivan}, M. and {Tendulkar}, S.~P. and {Yaron}, O.},
doi = {10.1111/j.1365-2966.2011.20240.x},
eprint = {1103.0779},
journal = {\mnras},
keywords = {accretion, accretion discs, black hole physics, galaxies: active, galaxies: nuclei},
month = {mar},
pages = {2684-2699},
primaryclass = {astro-ph.HE},
title = {{PTF10iya: a short-lived, luminous flare from the nuclear region of a star-forming galaxy}},
volume = {420},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2011.20240.x},
}
@article{2012ApJ...748...35S,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...748...35S},
archiveprefix = {arXiv},
author = {{Shen}, K.~J. and {Bildsten}, L. and {Kasen}, D. and {Quataert}, E.},
doi = {10.1088/0004-637X/748/1/35},
eid = {35},
eprint = {1108.4036},
journal = {\apj},
keywords = {binaries: close, nuclear reactions, nucleosynthesis, abundances, supernovae: general, white dwarfs},
month = {mar},
pages = {35, 10pp},
primaryclass = {astro-ph.HE},
title = {{The Long-term Evolution of Double White Dwarf Mergers}},
volume = {748},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/748/1/35},
}
@article{2012PASP..124...62O,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012PASP..124...62O},
archiveprefix = {arXiv},
author = {{Ofek}, E.~O. and {Laher}, R. and {Law}, N. and {Surace}, J. and {Levitan}, D. and {Sesar}, B. and {Horesh}, A. and {Poznanski}, D. and {van Eyken}, J.~C. and {Kulkarni}, S.~R. and {Nugent}, P. and {Zolkower}, J. and {Walters}, R. and {Sullivan}, M. and {Ag{\"u}eros}, M. and {Bildsten}, L. and {Bloom}, J. and {Cenko}, S.~B. and {Gal-Yam}, A. and {Grillmair}, C. and {Helou}, G. and {Kasliwal}, M.~M. and {Quimby}, R.},
doi = {10.1086/664065},
eprint = {1112.4851},
journal = {\pasp},
keywords = {Data Analysis and Techniques},
month = {jan},
pages = {62-73},
primaryclass = {astro-ph.IM},
title = {{The Palomar Transient Factory Photometric Calibration}},
volume = {124},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1086/664065},
}
@article{2012PASP..124....1S,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012PASP..124....1S},
archiveprefix = {arXiv},
author = {{Steinfadt}, J.~D.~R. and {Bildsten}, L. and {Kaplan}, D.~L. and {Fulton}, B.~J. and {Howell}, S.~B. and {Marsh}, T.~R. and {Ofek}, E.~O. and {Shporer}, A.},
doi = {10.1086/663865},
eprint = {1105.0472},
journal = {\pasp},
keywords = {Stars},
month = {jan},
pages = {1-13},
primaryclass = {astro-ph.SR},
title = {{A Search for Pulsations in Helium White Dwarfs}},
volume = {124},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1086/663865},
}
@article{2012ApJ...744L...6B,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...744L...6B},
archiveprefix = {arXiv},
author = {{Bildsten}, L. and {Paxton}, B. and {Moore}, K. and {Macias}, P.~J.},
doi = {10.1088/2041-8205/744/1/L6},
eid = {L6},
eprint = {1111.6867},
journal = {\apjl},
keywords = {stars: interiors, stars: late-type, stars: oscillations},
month = {jan},
pages = {L6, 5pp},
primaryclass = {astro-ph.SR},
title = {{Acoustic Signatures of the Helium Core Flash}},
volume = {744},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/744/1/L6},
}
@article{2011Natur.480..348L,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011Natur.480..348L},
archiveprefix = {arXiv},
author = {{Li}, W. and {Bloom}, J.~S. and {Podsiadlowski}, P. and {Miller}, A.~A. and {Cenko}, S.~B. and {Jha}, S.~W. and {Sullivan}, M. and {Howell}, D.~A. and {Nugent}, P.~E. and {Butler}, N.~R. and {Ofek}, E.~O. and {Kasliwal}, M.~M. and {Richards}, J.~W. and {Stockton}, A. and {Shih}, H.-Y. and {Bildsten}, L. and {Shara}, M.~M. and {Bibby}, J. and {Filippenko}, A.~V. and {Ganeshalingam}, M. and {Silverman}, J.~M. and {Kulkarni}, S.~R. and {Law}, N.~M. and {Poznanski}, D. and {Quimby}, R.~M. and {McCully}, C. and {Patel}, B. and {Maguire}, K. and {Shen}, K.~J.},
doi = {10.1038/nature10646},
eprint = {1109.1593},
journal = {\nat},
month = {dec},
pages = {348-350},
primaryclass = {astro-ph.CO},
title = {{Exclusion of a luminous red giant as a companion star to the progenitor of supernova SN 2011fe}},
volume = {480},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature10646},
}
@article{2011Natur.480..344N,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011Natur.480..344N},
archiveprefix = {arXiv},
author = {{Nugent}, P.~E. and {Sullivan}, M. and {Cenko}, S.~B. and {Thomas}, R.~C. and {Kasen}, D. and {Howell}, D.~A. and {Bersier}, D. and {Bloom}, J.~S. and {Kulkarni}, S.~R. and {Kandrashoff}, M.~T. and {Filippenko}, A.~V. and {Silverman}, J.~M. and {Marcy}, G.~W. and {Howard}, A.~W. and {Isaacson}, H.~T. and {Maguire}, K. and {Suzuki}, N. and {Tarlton}, J.~E. and {Pan}, Y.-C. and {Bildsten}, L. and {Fulton}, B.~J. and {Parrent}, J.~T. and {Sand}, D. and {Podsiadlowski}, P. and {Bianco}, F.~B. and {Dilday}, B. and {Graham}, M.~L. and {Lyman}, J. and {James}, P. and {Kasliwal}, M.~M. and {Law}, N.~M. and {Quimby}, R.~M. and {Hook}, I.~M. and {Walker}, E.~S. and {Mazzali}, P. and {Pian}, E. and {Ofek}, E.~O. and {Gal-Yam}, A. and {Poznanski}, D.},
doi = {10.1038/nature10644},
eprint = {1110.6201},
journal = {\nat},
month = {dec},
pages = {344-347},
primaryclass = {astro-ph.CO},
title = {{Supernova SN 2011fe from an exploding carbon-oxygen white dwarf star}},
volume = {480},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature10644},
}
@article{arnett_2010_aa,
abstract = {As a preliminary step toward a complete theoretical integration of three-dimensional compressible hydrodynamic simulations into stellar evolution, convection at the surface and sub-surface layers of the Sun is re-examined, from a restricted point of view, in the language of mixing-length theory (MLT). Requiring that MLT use a hydrodynamically realistic dissipation length gives a new constraint on solar models. While the stellar structure which results is similar to that obtained by Yale Rotational Evolution Code (Guenther et al.; Bahcall & Pinsonneault) and Garching models (Schlattl et al.), the theoretical picture differs. A new quantitative connection is made between macro-turbulence, micro-turbulence, and the convective velocity scale at the photosphere, which has finite values. The geometric parameter in MLT is found to correspond more reasonably with the thickness of the superadiabatic region (SAR), as it must for consistency in MLT, and its integrated effect may correspond to that of the strong downward plumes which drive convection (Stein & Nordlund), and thus has a physical interpretation even in MLT. If we crudely require the thickness of the SAR to be consistent with the geometric factor used in MLT, there is no longer a free parameter, at least in principle. Use of three-dimensional simulations of both adiabatic convection and stellar atmospheres will allow the determination of the dissipation length and the geometric parameter (i.e., the entropy jump) more realistically, and with no astronomical calibration. A physically realistic treatment of convection in stellar evolution will require substantial additional modifications beyond MLT, including nonlocal effects of kinetic energy flux, entrainment (the most dramatic difference from MLT found by Meakin & Arnett), rotation, and magnetic fields.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...710.1619A},
archiveprefix = {arXiv},
author = {{Arnett}, D. and {Meakin}, C. and {Young}, P.~A.},
date-added = {2013-02-06 04:29:29 +0000},
date-modified = {2013-02-06 04:29:29 +0000},
doi = {10.1088/0004-637X/710/2/1619},
eprint = {0910.0821},
journal = {\apj},
keywords = {binaries: eclipsing, convection, hydrodynamics, stars: atmospheres, stars: evolution, Sun: photosphere, white dwarfs},
month = {feb},
pages = {1619-1626},
primaryclass = {astro-ph.SR},
title = {{Convection Theory and Sub-Photospheric Stratification}},
volume = {710},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/710/2/1619},
}
@inproceedings{arnett_2010_ab,
abstract = {A program is outlined, and first results described, in which fully three-dimensional, time dependent simulations of hydrodynamic turbulence are used as a basis for theoretical investigation of the physics of turbulence. The inadequacy of the treatment of turbulent convection as a diffusive process is indicated. A generalization to rotation and magnetohydrodynamics is indicated, as are connections to simulations of 3D stellar atmospheres.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010IAUS..265..106A},
archiveprefix = {arXiv},
author = {{Arnett}, W.~D. and {Meakin}, C.},
booktitle = {Proc. IAU Symp. 265},
date-added = {2013-02-06 04:29:29 +0000},
date-modified = {2013-02-06 04:29:29 +0000},
doi = {10.1017/S174392131000030X},
editor = {{Cunha}, K. and {Spite}, M. and {Barbuy}, B.},
eprint = {0912.2978},
keywords = {turbulence, convection, hydrodynamics, rotation, waves, nucleosynthesis, plasma, stars: supernovae, stars: evolution},
month = {mar},
pages = {106-110},
primaryclass = {astro-ph.SR},
title = {{Turbulent Mixing in Stars: Theoretical Hurdles}},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1017/S174392131000030X},
}
@article{meakin_2011_aa,
abstract = {Issues concerning the structure and evolution of core collapse progenitor stars, and stellar evolution in general, are discussed with an emphasis on interior evolution. We discuss some recent results that address quantifying the uncertainties inherent in modern stellar evolution calculations, and we describe a research effort aimed at investigating the transport and mixing processes associated with stellar turbulence, which is arguably the greatest source of uncertainty in supernova progenitor structure, besides mass loss, at the time of core collapse. We highlight the important role played by precision observations of stellar parameters in constraining theoretical models, as well as the physical insight that can be garnered from three-dimensional hydrodynamic simulation.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011Ap%26SS.336..123M},
archiveprefix = {arXiv},
author = {{Meakin}, C.~A. and {Sukhbold}, T. and {Arnett}, W.~D.},
date-added = {2013-02-06 04:25:13 +0000},
date-modified = {2013-02-06 04:25:13 +0000},
doi = {10.1007/s10509-010-0591-8},
eprint = {1006.0513},
journal = {\apss},
keywords = {Convection, Stars: interiors, Turbulence},
month = {nov},
pages = {123-128},
primaryclass = {astro-ph.SR},
title = {{Presupernova structure of massive stars}},
volume = {336},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1007/s10509-010-0591-8},
}
@article{smartt_2009_aa,
abstract = {Knowledge of the progenitors of core-collapse supernovae is a fundamental component in understanding the explosions. The recent progress in finding such stars is reviewed. The minimum initial mass that can produce a supernova (SN) has converged to 8 $\pm$ 1 M from direct detections of red supergiant progenitors of II-P SNe and the most massive white dwarf progenitors, although this value is model dependent. It appears that most type Ibc SNe arise from moderate mass interacting binaries. The highly energetic, broad-lined Ic SNe are likely produced by massive, Wolf-Rayet progenitors. There is some evidence to suggest that the majority of massive stars above 20 M may collapse quietly to black holes and that the explosions remain undetected. The recent discovery of a class of ultrabright type II SNe and the direct detection of some progenitor stars bearing luminous blue variable characteristics suggest some very massive stars do produce highly energetic explosions. The physical mechanism is under debate, and these SNe pose a challenge to stellar evolutionary theory.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ARA%26A..47...63S},
archiveprefix = {arXiv},
author = {{Smartt}, S.~J.},
date-added = {2013-02-05 07:54:20 +0000},
date-modified = {2013-02-05 07:54:20 +0000},
doi = {10.1146/annurev-astro-082708-101737},
eprint = {0908.0700},
journal = {\araa},
month = {sep},
pages = {63-106},
primaryclass = {astro-ph.SR},
title = {{Progenitors of Core-Collapse Supernovae}},
volume = {47},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1146/annurev-astro-082708-101737},
}
@article{timmes_1994_aa,
abstract = {We determine the speeds, and many other physical properties, of flame fronts that propagate inward into degenerate and semidegenerate cores of carbon and oxygen (CO) and neon and oxygen (NeOMg) white dwarfs when such flames are bounded on their exterior by a convective region. Combustion in such fronts, per se, is incomplete, with only a small part of the initial mass function burned. A condition of balanced power is set up in the star where the rate of energy emitted as neutrinos from the convective region equals the power available from the unburned fuel that crosses the burning front. The propagation of the burning front itself is in turn limited by the temperature at the base of the convective shell, while cannot greatly exceed the adiabatic value. Solving for consistency between these two conditions gives a unique speed for the flame. Typical values for CO white dwarfs are a few hundredths of a centimeter per second. Flames in NeOMg mixtures are slower. Tables are presented in a form that can easily be implemented in stellar evolution codes and yield the rate at which the convective shell advances into the interior. Combining these velocities with the local equations for stellar structure, we find a minimum density for each gravitational potential below with the local equations for stellar structure, we find a minimum density for each gravitational potential below which the flame cannot propagate, and must die. Although detailed stellar models will have to be constructed to resolve some issues conclusively, our results that a CO white dwarf inginted at its edge will not burn carbon all the way to its center unless the mass of the white dwarf exceeds 0.8 solar mass. On the other hand, it is difficult to ignite carbon burning by compression alone anywhere in a white dwarf whose mass does not exceed 1.0 solar mass. Thus, compressionally ignited shell carbon burning in an accreting CO dwarf almost certainly propagates all the way to the center of the star. Implications for neutron star formation, and Type Ia supernova models, are briefly discussed. These are also applicable to massive stars in the about 10-12 solar mass range which ignite neon burning off center.},
adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1994ApJ...420..348T},
author = {{Timmes}, F.~X. and {Woosley}, S.~E. and {Taam}, R.~E.},
date-added = {2013-02-05 07:50:13 +0000},
date-modified = {2013-02-05 07:55:13 +0000},
journal = {\apj},
month = {jan},
pages = {348-363},
title = {{The conductive propagation of nuclear flames. 2: Convectively bounded flames in C + O and O + NE + MG cores}},
volume = {420},
year = {1994},
}
@article{timmes_1992_aa,
abstract = {The paper determines the physical properties - speed, width, and density structure - of conductive burning fronts in degenerate carbon-oxygen (C + O) and oxygen-neon-magnesium (O + Ne + Mg) compositions for a grid of initial densities and compositions. The dependence of the physical properties of the flame on the assumed values of nuclear reaction rates, the nuclear reaction network employed, the thermal conductivity, and the choice of coordinate system are investigated. The occurrence of accretion-induced collapse of a white dwarf is found to be critically dependent on the velocity of the nuclear conductive burning front and the growth rate of hydrodynamic instabilities. Treating the expanding area of the turbulent burning region as a fractal whose tile size is identical to the minimum unstable Rayleigh-Taylor wavelength, it is found, for all reasonable values of the fractal dimension, that for initial C + O or O + Ne + Mg densities above about 9 x 10 exp 9 g/cu cm the white dwarf should collapse to a neutron star.},
adsnote = {Provided by the Smithsonian/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1992ApJ...396..649T},
author = {{Timmes}, F.~X. and {Woosley}, S.~E.},
date-added = {2013-02-05 07:50:07 +0000},
date-modified = {2013-02-05 07:50:07 +0000},
journal = {\apj},
month = {sep},
pages = {649-667},
title = {{The conductive propagation of nuclear flames. I - Degenerate C + O and O + NE + MG white dwarfs}},
volume = {396},
year = {1992},
}
@article{eldridge_2004_aa,
abstract = {We present maps of the nature of single star progenitors of supernovae and their remnants in mass and metallicity space. We find our results are similar to others but we have gone further in varying the amount of mixing and using various mass-loss schemes to see how the maps change. We find that extra mixing, in the form of convective overshooting, moves boundaries such as the minimum mass for a supernova or Wolf-Rayet (WR) star to lower masses. We also find that the pre-WR mass loss determines the shape of our maps. We find that different mass-loss rates lead to quite different results. We find that the rise in luminosity at second dredge-up places quite tight constraints on the masses of some progenitors and in particular the progenitor of supernova 2003gd.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2004MNRAS.353...87E},
author = {{Eldridge}, J.~J. and {Tout}, C.~A.},
date-added = {2013-02-05 07:41:37 +0000},
date-modified = {2013-02-05 07:41:37 +0000},
doi = {10.1111/j.1365-2966.2004.08041.x},
eprint = {arXiv:astro-ph/0405408},
journal = {\mnras},
keywords = {stars: evolution, supernovae: general, supernovae: individual: SN 2003gd, stars: Wolf-Rayet},
month = {sep},
pages = {87-97},
title = {{The progenitors of core-collapse supernovae}},
volume = {353},
year = {2004},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2004.08041.x},
}
@article{nomoto_1988_aa,
abstract = {Not Available},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1988PhR...163...13N},
author = {{Nomoto}, K. and {Hashimoto}, M.},
date-added = {2013-02-05 07:35:23 +0000},
date-modified = {2013-02-05 07:35:23 +0000},
doi = {10.1016/0370-1573(88)90032-4},
journal = {\physrep},
keywords = {Massive Stars:Stellar Evolution, Presupernovae:Stellar Evolution, Stellar Evolution:Massive Stars, Stellar Evolution:Presupernovae},
pages = {13-36},
title = {{Presupernova evolution of massive stars.}},
volume = {163},
year = {1988},
bdsk-url-1 = {http://dx.doi.org/10.1016/0370-1573(88)90032-4},
}
@article{wanajo_2011_aa,
abstract = {We examine electron-capture supernovae (ECSNe) as sources of elements heavier than iron in the solar system and in Galactic halo stars. Nucleosynthesis calculations are performed on the basis of thermodynamic histories of mass elements from a fully self-consistent, two-dimensional hydrodynamic explosion model of an ECSN. We find that neutron-rich convective lumps with an electron fraction down to Y e,min = 0.40, which are absent in the one-dimensional counterpart, allow for interesting production of elements between the iron group and N = 50 nuclei (from Zn to Zr, with little Ga) in nuclear (quasi-)equilibrium. Our models yield very good agreement with the Ge, Sr, Y, and Zr abundances of r-process-deficient Galactic halo stars and constrain the occurrence of ECSNe to ~4% of all stellar core-collapse events. If tiny amounts of additional material with slightly lower Y e,min down to ~0.30-0.35 were also ejected---which presently cannot be excluded because of the limitations of resolution and two dimensionality of the model---a weak r-process can yield elements beyond N = 50 up to Pd, Ag, and Cd as observed in the r-process-deficient stars.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...726L..15W},
archiveprefix = {arXiv},
author = {{Wanajo}, S. and {Janka}, H.-T. and {M{\"u}ller}, B.},
date-added = {2013-02-05 07:32:56 +0000},
date-modified = {2013-02-05 07:49:57 +0000},
doi = {10.1088/2041-8205/726/2/L15},
eid = {L15},
eprint = {1009.1000},
journal = {\apjl},
keywords = {nuclear reactions, nucleosynthesis, abundances, stars: abundances, stars: neutron, supernovae: general},
month = {jan},
pages = {L15, 4pp},
primaryclass = {astro-ph.SR},
title = {{Electron-capture Supernovae as The Origin of Elements Beyond Iron}},
volume = {726},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/726/2/L15},
}
@article{fischer_2010_aa,
abstract = {Massive stars end their lives in explosions with kinetic energies on the order of 1051 erg. Immediately after the explosion has been launched, a region of low density and high entropy forms behind the ejecta, which is continuously subject to neutrino heating. The neutrinos emitted from the remnant at the center, the protoneutron star (PNS), heat the material above the PNS surface. This heat is partly converted into kinetic energy, and the material accelerates to an outflow that is known as the neutrino-driven wind. For the first time we simulate the collapse, bounce, explosion, and the neutrino-driven wind phases consistently over more than 20 s. Our numerical model is based on spherically symmetric general relativistic radiation hydrodynamics using spectral three-flavor Boltzmann neutrino transport. In simulations where no explosions are obtained naturally, we model neutrino-driven explosions for low- and intermediate-mass Fe-core progenitor stars by enhancing the charged current reaction rates. In the case of a special progenitor star, the 8.8 M_&sun; O-Ne-Mg-core, the explosion in spherical symmetry was obtained without enhanced opacities. The post-explosion evolution is in qualitative agreement with static steady-state and parametrized dynamic models of the neutrino-driven wind. On the other hand, we generally find lower neutrino luminosities and mean neutrino energies, as well as a different evolutionary behavior of the neutrino luminosities and mean neutrino energies. The neutrino-driven wind is proton-rich for more than 10 s and the contraction of the PNS differs from the assumptions made for the conditions at the inner boundary in previous neutrino-driven wind studies. Despite the moderately high entropies of about 100 kB/baryon and the fast expansion timescales, the conditions found in our models are unlikely to favor r-process nucleosynthesis. The simulations are carried out until the neutrino-driven wind settles down to a quasi-stationary state. About 5 s after the bounce, the peak temperature inside the PNS already starts to decrease because of the continued deleptonization. This moment determines the beginning of a cooling phase dominated by the emission of neutrinos. We discuss the physical conditions of the quasi-static PNS evolution and take the effects of deleptonization and mass accretion from early fallback into account.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...517A..80F},
archiveprefix = {arXiv},
author = {{Fischer}, T. and {Whitehouse}, S.~C. and {Mezzacappa}, A. and {Thielemann}, F.-K. and {Liebend{\"o}rfer}, M.},
date-added = {2013-02-05 07:28:01 +0000},
date-modified = {2013-02-05 07:28:01 +0000},
doi = {10.1051/0004-6361/200913106},
eid = {A80},
eprint = {0908.1871},
journal = {\aap},
keywords = {hydrodynamics, neutrinos, radiative transfer, relativistic processes},
month = {jul},
pages = {A80, 25pp},
primaryclass = {astro-ph.HE},
title = {{Protoneutron star evolution and the neutrino-driven wind in general relativistic neutrino radiation hydrodynamics simulations}},
volume = {517},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/200913106},
}
@article{kitaura_2006_aa,
abstract = {We present results of simulations of stellar collapse and explosions in spherical symmetry for progenitor stars in the 8-10 M_&sun; range with an O-Ne-Mg core. The simulations were continued until nearly one second after core bounce and were performed with the Prometheus/Vertex code with a variable Eddington factor solver for the neutrino transport, including a state-of-the-art treatment of neutrino-matter interactions. Particular effort was made to implement nuclear burning and electron capture rates with sufficient accuracy to ensure a smooth continuation, without transients, from the progenitor evolution to core collapse. Using two different nuclear equations of state (EoSs), a soft version of the Lattimer & Swesty EoS and the significantly stiffer Wolff & Hillebrandt EoS, we found no prompt explosions, but instead delayed explosions, powered by neutrino heating and the neutrino-driven baryonic wind which sets in about 200 ms after bounce. The models eject little nickel (< 0.015 M_&sun;), explode with an energy of ‚{\texttrademark}{\"U}0.1√{\'o} 1051 erg, and leave behind neutron stars (NSs) with a baryonic mass near 1.36 M_&sun;. Different from previous models of such explosions, the ejecta during the first second have a proton-to-baryon ratio of Ye ‚{\texttrademark}{\"U} 0.46, which suggests a chemical composition that is not in conflict with galactic abundances. No low-entropy matter with Ye ‚{\^a}{\texttrademark} 0.5 is ejected. This excludes such explosions as sites of a low-entropy r-process. The low explosion energy and nucleosynthetic implications are compatible with the observed properties of the Crab supernova, and the small nickel mass supports the possibility that our models explain some subluminous type II-P supernovae.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2006A%26A...450..345K},
author = {{Kitaura}, F.~S. and {Janka}, H.-T. and {Hillebrandt}, W.},
date-added = {2013-02-05 07:26:17 +0000},
date-modified = {2013-02-05 07:26:17 +0000},
doi = {10.1051/0004-6361:20054703},
eprint = {arXiv:astro-ph/0512065},
journal = {\aap},
keywords = {stars: supernovae: general, stars: supernovae: individual: Crab, neutrinos, hydrodynamics, radiative transfer},
month = {apr},
pages = {345-350},
title = {{Explosions of O-Ne-Mg cores, the Crab supernova, and subluminous type II-P supernovae}},
volume = {450},
year = {2006},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20054703},
}
@article{eldridge_2007_aa,
abstract = {We calculate the predicted UBVRIJHK absolute magnitudes for models of supernova progenitors and apply the result to the case of supernova 2005cs. We agree with previous results that the initial mass of the star was low, around 6 to 8 Msolar. However, such stars are thought to go through a second dredge-up to become asymptotic giant branch (AGB) stars. We show that had this occurred to the progenitor of 2005cs it would have been observed in JHK pre-explosion images. The progenitor was not detected in these bands and therefore we conclude that it was not an AGB star. Furthermore, if some AGB stars do produce supernovae they will have a clear signature in pre-explosion near-infrared images. Electron-capture supernovae are thought to occur in AGB stars, hence the implication is that 2005cs was not an electron-capture supernova but was the collapse of an iron core.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2007MNRAS.376L..52E},
author = {{Eldridge}, J.~J. and {Mattila}, S. and {Smartt}, S.~J.},
date-added = {2013-02-05 07:23:48 +0000},
date-modified = {2013-02-05 07:23:48 +0000},
doi = {10.1111/j.1745-3933.2007.00285.x},
eprint = {arXiv:astro-ph/0701152},
journal = {\mnras},
keywords = {stars: AGB and post-AGB, stars: evolution, supernovae: general, supernovae: individual: 2005cs, infrared: stars},
month = {mar},
pages = {L52-L56},
title = {{Ruling out a massive asymptotic giant-branch star as the progenitor of supernova 2005cs}},
volume = {376},
year = {2007},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1745-3933.2007.00285.x},
}
@article{wanajo_2009_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...695..208W},
archiveprefix = {arXiv},
author = {{Wanajo}, S. and {Nomoto}, K. and {Janka}, H.-T. and {Kitaura}, F.~S. and {M{\"u}ller}, B.},
date-added = {2013-02-05 07:21:15 +0000},
date-modified = {2013-02-05 07:21:15 +0000},
doi = {10.1088/0004-637X/695/1/208},
eprint = {0810.3999},
journal = {\apj},
keywords = {nuclear reactions, nucleosynthesis, abundances, stars: abundances, supernovae: general, supernovae: individual: SN 1054 SN 1997D SN 2008S},
month = {apr},
pages = {208-220},
title = {{Nucleosynthesis in Electron Capture Supernovae of Asymptotic Giant Branch Stars}},
volume = {695},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/695/1/208},
}
@article{nomoto_1982_aa,
abstract = {The initial mass of the Crab Nebula's progenitor star is estimated by comparing the observed nebular chemical abundances with detailed evolutionary calculations for 2.4- and 2.6-solar-mass helium cores of stars with masses of 8 to 10 solar masses. The results indicate that the mass of the Crab's progenitor was between the upper limit of about 8 solar masses for carbon deflagration and the lower limit of about 9.5 solar masses set by the dredge-up of the helium layer before the development of the helium-burning convective region. A scenario is outlined for the evolution of the progenitor star. It is suggested that the Crab Nebula was probably the product of an electron-capture supernova.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1982Natur.299..803N},
author = {{Nomoto}, K. and {Sugimoto}, D. and {Sparks}, W.~M. and {Fesen}, R.~A. and {Gull}, T.~R. and {Miyaji}, S.},
date-added = {2013-02-05 07:20:43 +0000},
date-modified = {2013-02-05 07:49:53 +0000},
doi = {10.1038/299803a0},
journal = {\nat},
keywords = {CRAB NEBULA, HELIUM, NUCLEAR FUSION, STELLAR EVOLUTION, STELLAR MASS, ABUNDANCE, CARBON, ELECTRON CAPTURE},
month = {oct},
pages = {803-805},
title = {{The Crab Nebula's progenitor}},
volume = {299},
year = {1982},
bdsk-url-1 = {http://dx.doi.org/10.1038/299803a0},
}
@article{davidson_1982_aa,
abstract = {Ultraviolet spectroscopy of the Crab Nebula done by the International Ultraviolet Explorer satellite is described, and an estimate of the carbon abundance is made, noting data reduction to remove spectral defects caused by radiation hits. The important C IV 1549, He II 1640, and semiforbidden C III 1908 emission line intensities were measured and upper limits placed on other ultraviolet features for the brightest filamentary region in the Nebula. The emission lines imply an average ionic abundance ratio n(C+2)/n(O+2) in the range from 0.4 to 1.5 in the observed gaseous condensations. The elemental abundance ratio of carbon to oxygen is probably in the same range. Analysis shows that there is no perceptible excess of carbon due to presupernova nucleosynthesis in the observed region. The large helium abundance, small carbon and oxygen abundances, and presence of a neutron star in the Crab Nebula suggest that the presupernova star had a mass close to eight solar masses.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1982ApJ...253..696D},
author = {{Davidson}, K. and {Gull}, T.~R. and {Maran}, S.~P. and {Stecher}, T.~P. and {Fesen}, R.~A. and {Parise}, R.~A. and {Harvel}, C.~A. and {Kafatos}, M. and {Trimble}, V.~L.},
date-added = {2013-02-05 07:19:00 +0000},
date-modified = {2013-02-05 07:19:00 +0000},
doi = {10.1086/159670},
journal = {\apj},
keywords = {ABUNDANCE, CARBON, CRAB NEBULA, IUE, SUPERNOVA REMNANTS, ULTRAVIOLET SPECTRA, EMISSION SPECTRA, HELIUM, MAIN SEQUENCE STARS, NEUTRON STARS, OXYGEN, STELLAR MASS, ULTRAVIOLET SPECTROPHOTOMETERS},
month = {feb},
pages = {696-706},
title = {{The ultraviolet spectrum of the Crab Nebula}},
volume = {253},
year = {1982},
bdsk-url-1 = {http://dx.doi.org/10.1086/159670},
}
@article{poelarends_2008_aa,
abstract = {We study the late evolution of solar metallicity stars in the transition region between white dwarf formation and core collapse. This includes the super-asymptotic giant branch (super-AGB, SAGB) stars, which ignite carbon burning and form an oxygen-neon (ONe) core. SAGB star cores may grow to the Chandrasekhar mass because of continued H- and He-shell burning, ending as core-collapse supernovae. From stellar evolution models we find that the initial mass range for SAGB evolution is 7.5-9.25 Msolar. We perform calculations with three different stellar evolution codes to judge the robustness of our results. The mass range significantly depends on the treatment of semiconvective mixing and convective overshooting. To consider the effect of a large number of thermal pulses, as expected in SAGB stars, we construct synthetic SAGB models that are calibrated through stellar evolution simulations. The synthetic model enables us to compute the evolution of the main properties of SAGB stars from the onset of thermal pulses until the core reaches the Chandrasekhar mass or is uncovered by the stellar wind. Thereby, we differentiate the stellar initial mass ranges that produce ONe WDs from that leading to electron-capture SNe. The latter is found to be 9.0-9.25 Msolar for our fiducial model, implying that electron-capture SNe would constitute about 4% of all SNe in the local universe. The error in this determination due to uncertainties in the third dredge-up efficiency and AGB mass-loss rate could lead to about a doubling of the number of electron-capture SNe, which provides a firm upper limit to their contribution to all supernovae of ~20%.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008ApJ...675..614P},
archiveprefix = {arXiv},
author = {{Poelarends}, A.~J.~T. and {Herwig}, F. and {Langer}, N. and {Heger}, A.},
date-added = {2013-02-05 07:16:42 +0000},
date-modified = {2013-02-05 07:16:42 +0000},
doi = {10.1086/520872},
eprint = {0705.4643},
journal = {\apj},
keywords = {Stars: AGB and Post-AGB, Stars: Evolution, Stars: Neutron, Stars: Supernovae: General},
month = {mar},
pages = {614-625},
title = {{The Supernova Channel of Super-AGB Stars}},
volume = {675},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1086/520872},
}
@article{ritossa_1999_aa,
abstract = {A stellar model of mass 11 M_solar and Population I composition is evolved from the hydrogen-burning main sequence through the core carbon-burning phase. In contrast with 9, 10, and 10.5 M_solar models studied in earlier papers of this series, carbon burning is ignited at the center of the 11 M_solar model. Like the 10.5 M_solar model, the 11 M_solar model experiences a dredge-out episode at the end of the carbon-burning phase. At the beginning of this episode, a semiconvective zone forms at the base of the hydrogen-rich envelope and carries hydrogen inward in mass toward the outer edge of a fully convective zone that is sustained by helium burning at its base. Hydrogen diffuses into the helium-rich convective zone untila hydrogen shell flash occurs. Helium burning dies out and the outer edge of the convective layer,sustained by fluxes due to hydrogen burning, extends outward in mass through hydrogen-rich material, mixing freshly synthesized nuclei outward. Then, hydrogen burning dies out and the outer edge of the convective shell, now sustained primarily by fluxes due to the release of gravothermal energy, moves outward until it reaches the inner edge of the convective envelope. Freshly synthesized material is then convected to the surface. Mixing during the final phase of homogenization in the convective envelope is maintained by fluxes due to the release of gravothermal energy. At the end of the dredge-out phase, the surface nitrogen abundance has decreased and the C/N ratio has changed from less than unity to larger than unity, showing that mixing has extended into regions where helium burning has manufactured substantial quantities of ^12C and destroyed ^14N. Prior to the dredge-out phase, neon burning is narrowly averted, and, after the dredge-out phase, neutrino losses due to electron capture and decay reactions between A=25 and A=23 isotopes in and above convective Urca shells cool the inner portions of the electron-degenerate oxygen-neon (ONe) core. Ultimately, the model becomes a thermally pulsing super-asymptotic giant branch (TPSAGB) star with an ONe core of mass ~1.368 M_solar. Hydrogen and helium burning over a period of ~1.4x10^4 yr of TPSAGB evolution add a carbon-oxygen layer of mass ~0.014 M_solar to the electron-degenerate core. Then, electron captures on products of carbon burning lead to the collapse of the core into a neutron star and expulsion of the envelope in a weak Type II supernova explosion. The ratio of helium to hydrogen in the ejecta is approximately twice solar.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1999ApJ...515..381R},
author = {{Ritossa}, C. and {Garc{\'{\i}}a-Berro}, E. and {Iben}, Jr., I.},
date-added = {2013-02-05 07:16:14 +0000},
date-modified = {2013-02-05 07:16:14 +0000},
doi = {10.1086/307017},
journal = {\apj},
keywords = {NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: ABUNDANCES, STARS: EVOLUTION, STARS: INTERIORS, STARS: SUPERGIANTS, STARS: SUPERNOVAE: GENERAL},
month = {apr},
pages = {381-397},
title = {{On the Evolution of Stars that Form Electron-degenerate Cores Processed by Carbon Burning. V. Shell Convection Sustained by Helium Burning, Transient Neon Burning, Dredge-out, URCA Cooling, and Other Properties of an 11 M\_solar Population I Model Star}},
volume = {515},
year = {1999},
bdsk-url-1 = {http://dx.doi.org/10.1086/307017},
}
@article{gutierrez_1996_aa,
abstract = {The final stages of the evolution of electron-degenerate ONeMg cores, resulting from carbon burning in `heavyweight intermediate-mass stars (8 M_{0 } M 10 M0) and growing in mass either from carbon burning in a shell or from accretion of matter in a close binary system, are examined. When due account is taken of the Coulomb corrections, both in the equation of state and in the electron capture threshold energies, explosive NeO ignition takes place at densities high enough to ensure gravitational collapse to nuclear matter densities. It is shown that this result holds for two extreme assumptions concerning mixing in the presence of an overstable temperature gradient: no mixing (Ledoux criterion) and ordinary convective entropy mixing according to the Schwarzschild criterion (the latter delaying explosive ignition to still higher densities). Discrepancies among earlier calculations, due to omission of Coulomb corrections, are clarified with the use of the most recent electron capture rates on the relevant nuclides plus very finely zoned models.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1996ApJ...459..701G},
author = {{Gutierrez}, J. and {Garcia-Berro}, E. and {Iben}, Jr., I. and {Isern}, J. and {Labay}, J. and {Canal}, R.},
date-added = {2013-02-05 07:15:43 +0000},
date-modified = {2013-02-05 07:15:43 +0000},
doi = {10.1086/176934},
journal = {\apj},
keywords = {NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: EVOLUTION, STARS: INTERIORS, STARS: SUPERGIANTS, STARS: WHITE DWARFS},
month = {mar},
pages = {701-705},
title = {{The Final Evolution of ONeMg Electron-Degenerate Cores}},
volume = {459},
year = {1996},
bdsk-url-1 = {http://dx.doi.org/10.1086/176934},
}
@article{nomoto_1987_aa,
abstract = {In this paper, the helium core of an 8.8 solar mass star is evolved from the helium-burning stage through the early stage of collapse of an O + Ne + Mg core. The star undergoes helium and carbon burning under nondegenerate conditions and leaves an O + Ne + Mg core. The penetration of the surface convection zone into the helium layer starts much earlier than in a 9.6 solar mass star studied elsewhere. The subsequent evolution is brought about by hydrogen-helium double-shell burning. The mass interior to the helium-burning shell, M(Heb), increases toward the Chandrasekhar limit. After M(Heb) reaches 1.375 solar mass, electron captures on Mg-24, Na-24, Ne-20, and F-20 take place. The electron concentration decreases, the resulting rapid core contraction ignites the oxygen deflagration, and the material undergoes incineration into nuclear statistical equilibrium at the oxygen deflagration front. The collapse of the core is accelerated, and the oxygen deflagration front advances.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1987ApJ...322..206N},
author = {{Nomoto}, K.},
date-added = {2013-02-05 07:13:49 +0000},
date-modified = {2013-02-05 07:13:49 +0000},
doi = {10.1086/165716},
journal = {\apj},
keywords = {ELECTRON CAPTURE, GRAVITATIONAL COLLAPSE, STELLAR CORES, STELLAR EVOLUTION, STELLAR MASS, SUPERNOVAE, CRAB NEBULA, NUCLEAR FUSION, STELLAR INTERIORS, STELLAR MODELS},
month = {nov},
pages = {206-214},
title = {{Evolution of 8-10 solar mass stars toward electron capture supernovae. II - Collapse of an O + NE + MG core}},
volume = {322},
year = {1987},
bdsk-url-1 = {http://dx.doi.org/10.1086/165716},
}
@article{lau_2012_aa,
abstract = {Context. The literature is rich in analysis and results related to thermally pulsing-asymptotic giant branch (TP-AGB) stars, but the problem of the instabilities that arise and cause the divergence of models during the late stages of their evolution is rarely addressed. Aims: We investigate the physical conditions, causes and consequences of the interruption in the calculations of massive AGB stars in the late thermally-pulsing AGB phase. Methods: We have thoroughly analysed the physical structure of a solar metallicity 8.5 M&sun; star and described the physical conditions at the base of the convective envelope (BCE) just prior to divergence. Results: We find that the local opacity maximum caused by M-shell electrons of Fe-group elements lead to the accumulation of an energy excess, to the departure of thermal equilibrium conditions at the base of the convective envelope and, eventually, to the divergence of the computed models. For the 8.5 M&sun; case we present in this work the divergence occurs when the envelope mass is about 2 M&sun;. The remaining envelope masses range between somewhat less than 1 and more than 2 M&sun; for stars with initial masses between 7 and 10 M&sun; and, therefore, our results are relevant for the evolution and yields of super-AGB stars. If the envelope is ejected as a consequence of the instability we are considering, the occurrence of electron-capture supernovae would be avoided at solar metallicity.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012A%26A...542A...1L},
archiveprefix = {arXiv},
author = {{Lau}, H.~H.~B. and {Gil-Pons}, P. and {Doherty}, C. and {Lattanzio}, J.},
date-added = {2013-02-05 07:12:43 +0000},
date-modified = {2013-02-05 07:12:43 +0000},
doi = {10.1051/0004-6361/201218826},
eid = {A1},
eprint = {1204.3931},
journal = {\aap},
keywords = {stars: AGB and post-AGB, stars: evolution, stars: winds, outflows, stars: interiors},
month = {jun},
pages = {A1, 9pp},
primaryclass = {astro-ph.SR},
title = {{The end of super AGB and massive AGB stars. I. The instabilities that determine the final mass of AGB stars}},
volume = {542},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201218826},
}
@article{doherty_2010_aa,
abstract = {We present an extensive set of detailed stellar models in the mass range 7.7-10.5 Msolar over the metallicity range Z = 10-5-0.02. These models were produced using the Monash University version of the Mount Stromlo Stellar Structure Program (MONSTAR) and follow the evolution from the pre-main sequence to the first thermal pulse of these super asymptotic giant branch stars. A quantitative comparison is made to the study of Siess. Prior to this study, only qualitative comparisons and code validations existed in this critical mass range, and the large variations in the literature were largely unexplained. The comparison presented here is particularly detailed due to the standardization of the input physics, where possible. The minimum initial mass of star which ignites carbon, Mup, was found to agree within 0.2Msolar between the codes over the entire metallicity range. We find exceptional agreement in the model results between these two codes for all stages of evolution up to and including carbon burning. For additional comparison, we also present results from the EVOLVE code, a modified version of the IBEN code as described in Gil-Pons, Guti{\'e}rrez & Garc{\'\i}a-Berro for some important variables during the carbon burning phase. Several numerical tests showed that the carbon burning phase is weakly dependent on the spatial resolution but that inadequate temporal resolution alters the behaviour of the convective zones. We also discovered that stars just below Mup may experience a carbon flash that is not followed by the development of the flame. Such aborted carbon burning models thus preserve a CO core surrounding by a 0.2-0.3Msolar shell of partially burnt carbon material. We present a simplified algorithm for calculating carbon burning that only relies on tracking two species, 12C and 16O, but which tests show works quite accurately for the a wide range of initial masses and compositions.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010MNRAS.401.1453D},
author = {{Doherty}, C.~L. and {Siess}, L. and {Lattanzio}, J.~C. and {Gil-Pons}, P.},
date-added = {2013-02-05 07:10:39 +0000},
date-modified = {2013-02-05 07:10:39 +0000},
doi = {10.1111/j.1365-2966.2009.15772.x},
journal = {\mnras},
keywords = {nuclear reactions, nucleosynthesis, abundances, methods: numerical, stars: AGB and post-AGB, stars: evolution},
month = {jan},
pages = {1453-1464},
title = {{Super asymptotic giant branch stars. I - Evolution code comparison}},
volume = {401},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1111/j.1365-2966.2009.15772.x},
}
@article{siess_2010_aa,
abstract = {Aims: We present the first simulations of the full evolution of super-AGB stars through the entire thermally pulsing AGB phase. We analyse their structural and evolutionary properties and determine the first SAGB yields. Methods: Stellar models of various initial masses and metallicities were computed using standard physical assumptions which prevents the third dredge-up from occurring. A postprocessing nucleosynthesis code was used to compute the SAGB yields, to quantify the effect of the third dredge-up (3DUP), and to assess the uncertainties associated with the treatment of convection. Results: Owing to their massive oxygen-neon core, SAGB stars suffer weak thermal pulses, have very short interpulse periods and develop very high temperatures at the base of their convective envelope (up to 140 × 108 K), leading to very efficient hot bottom burning. SAGB stars are consequently heavy manufacturers of 4He, 13C, and 14N. They are also able to inject significant amounts of 7Li, 17O, 25Mg, and 26,27Al in the interstellar medium. The 3DUP mainly affects the CNO yields, especially in the lower metallicity models. Our post-processing simulations also indicate that changes in the temperature at the base of the convective envelope, which would result from a change in the efficiency of convective energy transport, have a dramatic impact on the yields and represent another major source of uncertainty. Tables 2 to 6 are only available in electronic form at the CDS via anonymous ftp to cdsarc.u-strasbg.fr (130.79.128.5) or via http://cdsweb.u-strasbg.fr/cgi-bin/qcat?J/A+A/512/A10},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010A%26A...512A..10S},
author = {{Siess}, L.},
date-added = {2013-02-05 07:09:45 +0000},
date-modified = {2013-02-05 07:09:45 +0000},
doi = {10.1051/0004-6361/200913556},
eid = {A10},
journal = {\aap},
keywords = {stars: AGB and post-AGB, stars: evolution, nuclear reactions, nucleosynthesis, abundances, stars: abundances},
month = {mar},
pages = {A10, 13pp},
title = {{Evolution of massive AGB stars. III. the thermally pulsing super-AGB phase}},
volume = {512},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/200913556},
}
@article{siess_2007_aa,
abstract = {Context: Massive AGB (hereafter super-AGB or SAGB) stars ignite carbon off-center and have initial masses ranging between Mup, the minimum initial mass for carbon ignition, and M_mas the minimum mass for the formation of an iron core collapse supernova. In this mass interval, stars more massive than Mn will undergo an electron capture supernova (EC-SN). Aims: We study the fate and selected evolutionary properties of SAGB stars up to the end of the carbon burning phase as a function of metallicity and core overshooting. Methods: The method is based on the analysis of a large set of stellar models covering the mass range 5-13 M&sun; and calculated for 7 different metallicities between Z=10-5 and twice solar. Core overshooting was considered in two subsets for Z=10-4 and 0.02. The models are available online at http://www-astro.ulb.ac.be/ siess/database.html. The fate of SAGB stars is investigated through a parametric model which allows us to assess the role of mass loss and of the third dredge-up. Results: Our main results can be summarized as follows: a) prior to C-burning, the evolution of SAGB stars is very similar to that of intermediate-mass stars, being more luminous, b) SAGB stars suffer a large He enrichment at the end of the second dredge-up, c) the limiting masses Mup, Mn and M_mas present a nonlinear behavior with Z, characterized by a minimum around Z=10-4, d) the values of Mup, Mn and M_mas are decreased by 2 M&sun; when core overshooting is considered, e) our models predict a minimum oxygen-neon white dwarf mass of 1.05 M&sun;, f) the determination of Mn is highly dependent on the mass loss and core growth rates, g) the evolutionary channel for EC-SN is limited to a very narrow mass range of ‚{\texttrademark}{\"O}1-1.5 M&sun; width and this mass window can be further decreased if some metallicity scaling factor is applied to the mass loss rate, h) the final fate of SAGB stars is connected to the second dredge-up and this property allowed us to refine the initial mass range for the formation of EC-SN. We find that if the ratio of the mass loss rate to the core growth rate averaged over the post carbon-burning evolution zeta = |overline{dot M}_loss/overline{dot M}_core| is greater than about 70-90, the evolutionary path to EC-SN is not accessible. Tables 4 and 5 are only available in electronic form at http://www.aanda.org},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2007A%26A...476..893S},
author = {{Siess}, L.},
date-added = {2013-02-05 07:08:46 +0000},
date-modified = {2013-02-05 07:08:46 +0000},
doi = {10.1051/0004-6361:20078132},
journal = {\aap},
keywords = {stars: evolution, stars: AGB and post-AGB , stars: supernovae: general, stars: white dwarfs, stars:, mass-loss},
month = {dec},
pages = {893-909},
title = {{Evolution of massive AGB stars. II. model properties at non-solar metallicity and the fate of Super-AGB stars}},
volume = {476},
year = {2007},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20078132},
}
@article{garcia-berro_1997_aa,
author = {{Garcia-Berro}, E. and {Ritossa}, C. and {Iben}, Jr., I.},
title = {{On the Evolution of Stars That Form Electron-Degenerate Cores Processed by Carbon Burning. III. The Inward Propagation of a Carbon-burning Flame and Other Properties of a 9 M$_{sun}$ Model Star}},
journal = {\apj},
keywords = {NUCLEAR REACTIONS, NUCLEOSYNTHESIS, ABUNDANCES, STARS: EVOLUTION, STARS: INTERIORS, STARS: SUPERGIANTS, STARS: WHITE DWARFS},
year = {1997},
month = {aug},
volume = {485},
pages = {765-784},
doi = {10.1086/304444},
adsurl = {http://adsabs.harvard.edu/abs/1997ApJ...485..765G},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@article{nomoto_1984_aa,
abstract = {One triggering mechanism suggested for supernovae involves the collapse of a degenerate core due to electron captures. Barkat et al. (1974) showed that an eight solar mass star develops a degenerate core after nonexplosive carbon burning. Miyaji et al. (1980) performed hydrodynamical calculations regarding a degenerate O + Ne + Mg core. It was found that electron captures on Mg-24 and Ne-20 trigger the collapse of the core prior to the initiation of explosive oxygen burning. In the present investigation the gravitational contraction of hypothetical pure neon stars is discussed in order to clarify the effect of electron degeneracy on neon ignition and stellar evolution, which is crucial for 8-10 solar mass stars. A summary is provided of the evolution from helium burning through the phase of the developing O + Ne + Mg core. Attention is given to neon ignition, the origin of hydrogen-deficient carbon stars, and the evolution toward supernova stages, and possible formation of white dwarfs.},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1984ApJ...277..791N},
author = {{Nomoto}, K.},
date-added = {2013-02-05 07:05:18 +0000},
date-modified = {2013-02-05 07:05:25 +0000},
doi = {10.1086/161749},
journal = {\apj},
keywords = {ABUNDANCE, ELECTRON CAPTURE, STELLAR EVOLUTION, STELLAR STRUCTURE, SUPERNOVAE, CARBON STARS, GRAVITATIONAL COLLAPSE, MAGNESIUM, MILKY WAY GALAXY, NEON, NUCLEAR FUSION, OXYGEN, WHITE DWARF STARS},
month = {feb},
pages = {791-805},
title = {{Evolution of 8-10 solar mass stars toward electron capture supernovae. I - Formation of electron-degenerate O + NE + MG cores}},
volume = {277},
year = {1984},
bdsk-url-1 = {http://dx.doi.org/10.1086/161749},
}
@article{monnier10,
author = {{Monnier}, J.~D. and {Townsend}, R.~H.~D. and {Che}, X. and {Zhao}, M. and {Kallinger}, T. and {Matthews}, J. and {Moffat}, A.~F.~J.},
journal = {\apj},
month = {dec},
pages = {1192-1201},
title = {{Rotationally Modulated g-modes in the Rapidly Rotating {$\delta$} Scuti Star Rasalhague ({$\alpha$} Ophiuchi)}},
volume = {725},
year = {2010},
}
@article{alecian11,
author = {{Alecian}, E. and {Kochukhov}, O. and {Neiner}, C. and {Wade}, G.~A. and {de Batz}, B. and {Henrichs}, H. and {Grunhut}, J.~H. and {Bouret}, J.-C. and {Briquet}, M. and {Gagne}, M. and {Naze}, Y. and {Oksala}, M.~E. and {Rivinius}, T. and {Townsend}, R.~H.~D. and {Walborn}, N.~R. and {Weiss}, W. and {Mimes Collaboration}},
journal = {\aap},
month = {dec},
pages = {L6, 4pp},
title = {{First HARPSpol discoveries of magnetic fields in massive stars}},
volume = {536},
year = {2011},
}
@article{oksala12,
author = {{Oksala}, M.~E. and {Wade}, G.~A. and {Townsend}, R.~H.~D. and {Owocki}, S.~P. and {Kochukhov}, O. and {Neiner}, C. and {Alecian}, E. and {Grunhut}, J.},
journal = {\mnras},
month = {jan},
pages = {959-970},
title = {{Revisiting the Rigidly Rotating Magnetosphere model for {$\sigma$} Ori E - I. Observations and data analysis}},
volume = {419},
year = {2012},
}
@article{grunhut12,
archiveprefix = {arXiv},
author = {{Grunhut}, J.~H. and {Rivinius}, T. and {Wade}, G.~A. and {Townsend}, R.~H.~D. and {Marcolino}, W.~L.~F. and {Bohlender}, D.~A. and {Szeifert}, T. and {Petit}, V. and {Matthews}, J.~M. and {Rowe}, J.~F. and {Moffat}, A.~F.~J. and {Kallinger}, T. and {Kuschnig}, R. and {Guenther}, D.~B. and {Rucinski}, S.~M. and {Sasselov}, D. and {Weiss}, W.~W.},
journal = {\mnras},
month = {jan},
pages = {1610-1627},
title = {{HR 5907: Discovery of the most rapidly rotating magnetic early B-type star by the MiMeS Collaboration}},
volume = {419},
year = {2012},
}
@article{wade12,
author = {{Wade}, G.~A. and {Grunhut}, J. and {Gr{\"a}fener}, G. and {Howarth}, I.~D. and {Martins}, F. and {Petit}, V. and {Vink}, J.~S. and {Bagnulo}, S. and {Folsom}, C.~P. and {Naz{\'e}}, Y. and {Walborn}, N.~R. and {Townsend}, R.~H.~D. and {Evans}, C.~J.},
journal = {\mnras},
month = {jan},
pages = {2459-2471},
title = {{The spectral variability and magnetic field characteristics of the Of?p star HD 148937}},
volume = {419},
year = {2012},
}
@inproceedings{townsend09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009AIPC.1170..355T},
author = {{Townsend}, R.},
booktitle = {AIP Conf. Ser. 1170},
doi = {10.1063/1.3246512},
editor = {{Guzik}, J.~A. and {Bradley}, P.~A.},
keywords = {Cepheids, Hydrodynamics, Pulsations, oscillations, and stellar seismology},
month = {sep},
pages = {355-359},
title = {{Toward Self-consistent Angular Momentum Transport in Pulsating Massive Stars}},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1063/1.3246512},
}
@inproceedings{bard11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011AAS...21734214B},
author = {{Bard}, C. and {Teitler}, S.},
booktitle = {\aasabs\ 217},
date-modified = {2013-02-11 07:48:59 +0000},
month = {jan},
pages = {342.14},
title = {{A Novel Approach to Solve Linearized Stellar Pulsation Equations}},
volume = {43},
year = {2011},
}
@inproceedings{townsend12a,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012AIPC.1429..278T},
author = {{Townsend}, R.},
booktitle = {AIP Conf. Ser. 1429},
doi = {10.1063/1.3701941},
editor = {{Hoffman}, J.~L. and {Bjorkman}, J. and {Whitney}, B.},
month = {may},
pages = {278-281},
title = {{A Monte-Carlo method for simulating linear polarization variations in clumpy massive-star winds}},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1063/1.3701941},
}
@inproceedings{townsend12b,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ASPC..464..385T},
author = {{Townsend}, R.~H.~D.},
booktitle = {ASP Conf. Ser. 464},
editor = {{Carciofi}, A.~C. and {Rivinius}, T.},
month = {dec},
pages = {385-394},
title = {{Massive-Star Magnetospheres: The Interplay Between Outflows, Rotation and Magnetic Fields}},
year = {2012},
}
@inproceedings{carciofi12,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ASPC..464..413C},
author = {{Carciofi}, A.~C. and {Faes}, D.~M. and {Townsend}, R.~H.~D.},
booktitle = {ASP Conf. Ser. 464},
editor = {{Carciofi}, A.~C. and {Rivinius}, T.},
month = {dec},
pages = {413-422},
title = {{Polarimetric Observations of {$\sigma$} Orionis E}},
year = {2012},
}
@INPROCEEDINGS{hawley_2013_aa,
author = {{Hawley}, W. and {Timmes}, F.~X.},
title = {{Non-Zero Impact Parameter White Dwarf Collisions in FLASH}},
booktitle = {\aasabs\ 221},
year = {2013},
month = {jan},
pages = {253.27},
adsurl = {http://adsabs.harvard.edu/abs/2013AAS...22125327H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@inproceedings{timmes_2010_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010APS..DNP2WB003T},
author = {{Timmes}, F.},
booktitle = {APS Meeting Abstracts 55},
date-added = {2013-02-04 01:40:22 +0000},
date-modified = {2013-02-04 01:40:24 +0000},
month = {nov},
pages = {3},
title = {{Diagnostics for Thermonuclear and Core-Collapse Supernovae}},
year = {2010},
}
@INPROCEEDINGS{hawley_2011_aa,
author = {{Hawley}, W. and {Athanassiadou}, T. and {Raskin}, C. and {Richardson}, M. and {Scannapieco}, E. and {Timmes}, F.},
title = {{White Dwarf Collisions as Potential SNIa Progenitors}},
booktitle = {\aasabs\ 217},
year = {2011},
month = {jan},
pages = {341.09},
adsurl = {http://adsabs.harvard.edu/abs/2011AAS...21734109H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@inproceedings{de_2011_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011AAS...21743424D},
author = {{De}, S. and {Baron}, E. and {Timmes}, F. and {Hauschildt}, P.},
booktitle = {\aasabs\ 217},
date-added = {2013-02-04 01:29:25 +0000},
date-modified = {2013-02-11 07:50:15 +0000},
month = {jan},
pages = {434.24},
title = {{Radiative Transfer Calculation Of Light Curves And Spectra For Type Ia Sne Models}},
year = {2011},
}
@INPROCEEDINGS{hawley_2012_ab,
author = {{Hawley}, W. and {Athanassiadou}, T. and {Timmes}, F. and {Raskin}, C. and {Richardson}, M.},
title = {{White Dwarf Collisions: Grid versus Particle Codes}},
booktitle = {\aasabs\ 219},
year = {2012},
month = {jan},
pages = {436.05},
adsurl = {http://adsabs.harvard.edu/abs/2012AAS...21943605H},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@inproceedings{athanassiadou_2012_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012AAS...21943601A},
author = {{Athanassiadou}, T. and {Hawley}, W. and {Timmes}, F.},
booktitle = {\aasabs\ 219},
date-added = {2013-02-04 01:23:50 +0000},
date-modified = {2013-02-11 07:47:04 +0000},
month = {jan},
pages = {436.01},
title = {{Off-center Collisions of two White Dwarfs: A Type Ia Supernova Progenitor Scenario.}},
year = {2012},
}
@article{raskin_2009_ab,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009ApJ...707...74R},
archiveprefix = {arXiv},
author = {{Raskin}, C. and {Scannapieco}, E. and {Rhoads}, J. and {Della Valle}, M.},
date-added = {2013-02-04 01:18:45 +0000},
date-modified = {2013-02-04 01:18:45 +0000},
doi = {10.1088/0004-637X/707/1/74},
eprint = {0909.4293},
journal = {\apj},
keywords = {stars: evolution, supernovae: general},
month = {dec},
pages = {74-78},
primaryclass = {astro-ph.SR},
title = {{Prompt Ia Supernovae are Significantly Delayed}},
volume = {707},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/707/1/74},
}
@article{hawley_2012_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
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author = {{Hawley}, W.~P. and {Athanassiadou}, T. and {Timmes}, F.~X.},
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title = {{Zero Impact Parameter White Dwarf Collisions in FLASH}},
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@article{raskin_2012_aa,
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author = {{Raskin}, C. and {Scannapieco}, E. and {Fryer}, C. and {Rockefeller}, G. and {Diehl}, S. and {Timmes}, F.~X.},
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title = {{Remnants Of Binary White Dwarf Mergers}},
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@article{raskin_2010_aa,
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adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...724..111R},
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author = {{Raskin}, C. and {Scannapieco}, E. and {Rockefeller}, G. and {Fryer}, C. and {Diehl}, S. and {Timmes}, F.~X.},
date-added = {2013-02-04 01:16:24 +0000},
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doi = {10.1088/0004-637X/724/1/111},
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title = {{{56}Ni Production in Double-degenerate White Dwarf Collisions}},
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}
@article{raskin_2009_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009MNRAS.399L.156R},
archiveprefix = {arXiv},
author = {{Raskin}, C. and {Timmes}, F.~X. and {Scannapieco}, E. and {Diehl}, S. and {Fryer}, C.},
date-added = {2013-02-04 01:16:13 +0000},
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doi = {10.1111/j.1745-3933.2009.00743.x},
eprint = {0907.3915},
journal = {\mnras},
keywords = {hydrodynamics , nuclear reactions, nucleosynthesis, abundances , supernovae: general , white dwarfs},
month = {oct},
pages = {L156-L159},
title = {{On Type Ia supernovae from the collisions of two white dwarfs}},
volume = {399},
year = {2009},
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}
@article{metcalfe13,
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adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...763L..26M},
archiveprefix = {arXiv},
author = {{Metcalfe}, T.~S. and {Buccino}, A.~P. and {Brown}, B.~P. and {Mathur}, S. and {Soderblom}, D.~R. and {Henry}, T.~J. and {Mauas}, P.~J.~D. and {Petrucci}, R. and {Hall}, J.~C. and {Basu}, S.},
doi = {10.1088/2041-8205/763/2/L26},
eid = {L26},
eprint = {1212.4425},
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keywords = {stars: activity, stars: chromospheres, stars: individual: HD 22049, surveys},
month = {feb},
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title = {{Magnetic Activity Cycles in the Exoplanet Host Star epsilon Eridani}},
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year = {2013},
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}
@article{nelson13,
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adsurl = {http://adsabs.harvard.edu/abs/2013ApJ...762...73N},
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author = {{Nelson}, N.~J. and {Brown}, B.~P. and {Brun}, A.~S. and {Miesch}, M.~S. and {Toomre}, J.},
doi = {10.1088/0004-637X/762/2/73},
eid = {73},
eprint = {1211.3129},
journal = {\apj},
keywords = {convection, stars: interiors, stars: magnetic field, Sun: interior},
month = {jan},
pages = {73, 20pp},
primaryclass = {astro-ph.SR},
title = {{Magnetic Wreaths and Cycles in Convective Dynamos}},
volume = {762},
year = {2013},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/762/2/73},
}
@article{rahbarnia12,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...759...80R},
author = {{Rahbarnia}, K. and {Brown}, B.~P. and {Clark}, M.~M. and {Kaplan}, E.~J. and {Nornberg}, M.~D. and {Rasmus}, A.~M. and {Zane Taylor}, N. and {Forest}, C.~B. and {Jenko}, F. and {Limone}, A. and {Pinton}, J.-F. and {Plihon}, N. and {Verhille}, G.},
doi = {10.1088/0004-637X/759/2/80},
eid = {80},
journal = {\apj},
keywords = {dynamo, magnetohydrodynamics: MHD, methods: laboratory, turbulence},
month = {nov},
pages = {80, 6pp},
title = {{Direct Observation of the Turbulent emf and Transport of Magnetic Field in a Liquid Sodium Experiment}},
volume = {759},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/759/2/80},
}
@article{augustson12,
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adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...756..169A},
author = {{Augustson}, K.~C. and {Brown}, B.~P. and {Brun}, A.~S. and {Miesch}, M.~S. and {Toomre}, J.},
doi = {10.1088/0004-637X/756/2/169},
eid = {169},
journal = {\apj},
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month = {sep},
pages = {169, 23pp},
title = {{Convection and Differential Rotation in F-type Stars}},
volume = {756},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/756/2/169},
}
@article{brown12,
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adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...756..109B},
archiveprefix = {arXiv},
author = {{Brown}, B.~P. and {Vasil}, G.~M. and {Zweibel}, E.~G.},
doi = {10.1088/0004-637X/756/2/109},
eid = {109},
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primaryclass = {astro-ph.SR},
title = {{Energy Conservation and Gravity Waves in Sound-proof Treatments of Stellar Interiors. Part I. Anelastic Approximations}},
volume = {756},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/756/2/109},
}
@article{miesch12,
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adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...746L..26M},
archiveprefix = {arXiv},
author = {{Miesch}, M.~S. and {Brown}, B.~P.},
doi = {10.1088/2041-8205/746/2/L26},
eid = {L26},
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month = {feb},
pages = {L26, 5pp},
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title = {{Convective Babcock-Leighton Dynamo Models}},
volume = {746},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/746/2/L26},
}
@article{matt11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011AN....332..897M},
archiveprefix = {arXiv},
author = {{Matt}, S.~P. and {Do Cao}, O. and {Brown}, B.~P. and {Brun}, A.~S.},
doi = {10.1002/asna.201111624},
eprint = {1111.5585},
journal = {\an},
keywords = {convection, hydrodynamics, stars: interiors, stars: rotation, turbulence, methods: numerical},
month = {dec},
pages = {897-906},
primaryclass = {astro-ph.SR},
title = {{Convection and differential rotation properties of G and K stars computed with the ASH code}},
volume = {332},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1002/asna.201111624},
}
@article{nelson11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...739L..38N},
archiveprefix = {arXiv},
author = {{Nelson}, N.~J. and {Brown}, B.~P. and {Brun}, A.~S. and {Miesch}, M.~S. and {Toomre}, J.},
doi = {10.1088/2041-8205/739/2/L38},
eid = {L38},
eprint = {1108.4697},
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month = {oct},
pages = {L38, 5pp},
primaryclass = {astro-ph.SR},
title = {{Buoyant Magnetic Loops in a Global Dynamo Simulation of a Young Sun}},
volume = {739},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/2041-8205/739/2/L38},
}
@article{brown11,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2011ApJ...731...69B},
archiveprefix = {arXiv},
author = {{Brown}, B.~P. and {Miesch}, M.~S. and {Browning}, M.~K. and {Brun}, A.~S. and {Toomre}, J.},
doi = {10.1088/0004-637X/731/1/69},
eid = {69},
eprint = {1102.1993},
journal = {\apj},
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month = {apr},
pages = {69, 19pp},
primaryclass = {astro-ph.SR},
title = {{Magnetic Cycles in a Convective Dynamo Simulation of a Young Solar-type Star}},
volume = {731},
year = {2011},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/731/1/69},
}
@article{lecoanet10,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2010ApJ...712.1116L},
archiveprefix = {arXiv},
author = {{Lecoanet}, D. and {Zweibel}, E.~G. and {Townsend}, R.~H.~D. and {Huang}, Y.-M.},
doi = {10.1088/0004-637X/712/2/1116},
eprint = {1002.3335},
journal = {\apj},
keywords = {hydrodynamics, instabilities, magnetohydrodynamics: MHD, stars: magnetic field, stars: rotation},
month = {apr},
pages = {1116-1128},
primaryclass = {astro-ph.SR},
title = {{Violation of Richardson's Criterion Via Introduction of a Magnetic Field}},
volume = {712},
year = {2010},
bdsk-url-1 = {http://dx.doi.org/10.1088/0004-637X/712/2/1116},
}
@article{pantillon07,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2007A%26A...474..155P},
archiveprefix = {arXiv},
author = {{Pantillon}, F.~P. and {Talon}, S. and {Charbonnel}, C.},
doi = {10.1051/0004-6361:20078078},
eprint = {0708.1477},
journal = {\aap},
keywords = {hydrodynamics, turbulence, waves, methods: numerical, stars: interiors, stars: rotation},
month = {oct},
pages = {155-163},
title = {{Angular momentum transport by internal gravity waves. III. Wave excitation by core convection and the Coriolis effect}},
volume = {474},
year = {2007},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20078078},
}
@article{maeder87,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1987A%26A...178..159M},
author = {{Maeder}, A.},
journal = {\aap},
keywords = {BLUE STARS, STELLAR EVOLUTION, SUPERMASSIVE STARS, BAROCLINIC INSTABILITY, CRITICAL VELOCITY, MIXING, STELLAR ROTATION, STELLAR STRUCTURE, TURBULENT DIFFUSION, VISCOSITY},
month = {may},
pages = {159-169},
title = {{Evidences for a bifurcation in massive star evolution. The ON-blue stragglers}},
volume = {178},
year = {1987},
}
@article{fruchter06,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2006Natur.441..463F},
author = {{Fruchter}, A.~S. and {Levan}, A.~J. and {Strolger}, L. and {Vreeswijk}, P.~M. and {Thorsett}, S.~E. and {Bersier}, D. and {Burud}, I. and {Castro Cer{\'o}n}, J.~M. and {Castro-Tirado}, A.~J. and {Conselice}, C. and {Dahlen}, T. and {Ferguson}, H.~C. and {Fynbo}, J.~P.~U. and {Garnavich}, P.~M. and {Gibbons}, R.~A. and {Gorosabel}, J. and {Gull}, T.~R. and {Hjorth}, J. and {Holland}, S.~T. and {Kouveliotou}, C. and {Levay}, Z. and {Livio}, M. and {Metzger}, M.~R. and {Nugent}, P.~E. and {Petro}, L. and {Pian}, E. and {Rhoads}, J.~E. and {Riess}, A.~G. and {Sahu}, K.~C. and {Smette}, A. and {Tanvir}, N.~R. and {Wijers}, R.~A.~M.~J. and {Woosley}, S.~E.},
doi = {10.1038/nature04787},
eprint = {arXiv:astro-ph/0603537},
journal = {\nat},
month = {may},
pages = {463-468},
title = {{Long {$\gamma$}-ray bursts and core-collapse supernovae have different environments}},
volume = {441},
year = {2006},
bdsk-url-1 = {http://dx.doi.org/10.1038/nature04787},
}
@article{bondarescu09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009PhRvD..79j4003B},
archiveprefix = {arXiv},
author = {{Bondarescu}, R. and {Teukolsky}, S.~A. and {Wasserman}, I.},
doi = {10.1103/PhysRevD.79.104003},
eid = {104003},
eprint = {0809.3448},
journal = {\prd},
keywords = {Relativistic stars: structure, stability, and oscillations, Wave generation and sources, Pulsations, oscillations, and stellar seismology, Neutron stars},
month = {may},
number = {10},
pages = {104003, 22pp},
title = {{Spinning down newborn neutron stars: Nonlinear development of the r-mode instability}},
volume = {79},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1103/PhysRevD.79.104003},
}
@article{woosley93,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1993ApJ...405..273W},
author = {{Woosley}, S.~E.},
doi = {10.1086/172359},
journal = {\apj},
keywords = {ACCRETION DISKS, BLACK HOLES (ASTRONOMY), GAMMA RAY BURSTS, STELLAR EVOLUTION, STELLAR MASS ACCRETION, STELLAR PHYSICS, ASTRONOMICAL MODELS, SUPERNOVAE, WOLF-RAYET STARS},
month = {mar},
pages = {273-277},
title = {{Gamma-ray bursts from stellar mass accretion disks around black holes}},
volume = {405},
year = {1993},
bdsk-url-1 = {http://dx.doi.org/10.1086/172359},
}
@article{mathis08,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008SoPh..251..101M},
author = {{Mathis}, S. and {Talon}, S. and {Pantillon}, F.-P. and {Zahn}, J.-P.},
doi = {10.1007/s11207-008-9157-0},
journal = {\solphys},
keywords = {Hydrodynamics, Turbulence, Waves, Methods: numerical, Stars: interiors, Stars: rotation},
month = {sep},
pages = {101-118},
title = {{Angular Momentum Transport in the Sun's Radiative Zone by Gravito-Inertial Waves}},
volume = {251},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1007/s11207-008-9157-0},
}
@article{ott06,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2006ApJS..164..130O},
author = {{Ott}, C.~D. and {Burrows}, A. and {Thompson}, T.~A. and {Livne}, E. and {Walder}, R.},
doi = {10.1086/500832},
eprint = {arXiv:astro-ph/0508462},
journal = {\apjs},
keywords = {Hydrodynamics, Neutrinos, Stars: Pulsars: General, Radiative Transfer, Stars: Evolution, Stars: Neutron, Stars: Rotation, Stars: Supernovae: General},
month = {may},
pages = {130-155},
title = {{The Spin Periods and Rotational Profiles of Neutron Stars at Birth}},
volume = {164},
year = {2006},
bdsk-url-1 = {http://dx.doi.org/10.1086/500832},
}
@article{lyutikov01,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2001MNRAS.321..177L},
author = {{Lyutikov}, M. and {Blackman}, E.~G.},
doi = {10.1046/j.1365-8711.2001.04190.x},
eprint = {arXiv:astro-ph/0004212},
journal = {\mnras},
keywords = {RADIATION MECHANISMS: NON-THERMAL, GAMMA-RAYS: BURSTS, radiation mechanisms: non-thermal, gamma-rays: bursts},
month = {feb},
pages = {177-186},
title = {{Gamma-ray bursts from unstable Poynting-dominated outflows}},
volume = {321},
year = {2001},
bdsk-url-1 = {http://dx.doi.org/10.1046/j.1365-8711.2001.04190.x},
}
@article{zweibel89,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1989ApJ...343..994Z},
author = {{Zweibel}, E.~G. and {Daeppen}, W.},
doi = {10.1086/167768},
journal = {\apj},
keywords = {FIELD THEORY (PHYSICS), MAGNETOHYDRODYNAMIC WAVES, SOLAR INTERIOR, SOLAR MAGNETIC FIELD, SOLAR OSCILLATIONS, LORENTZ FORCE, MAGNETIC FLUX, PHOTOSPHERE},
month = {aug},
pages = {994-1003},
title = {{Effects of magnetic fibrils on solar oscillation frequencies - Mean field theory}},
volume = {343},
year = {1989},
bdsk-url-1 = {http://dx.doi.org/10.1086/167768},
}
@article{parker82,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1982ApJ...256..302P},
author = {{Parker}, E.~N.},
doi = {10.1086/159908},
journal = {\apj},
month = {may},
pages = {302-315},
title = {{The Dynamics of Fibril Magnetic Fields - Part Two - the Mean Field Equations}},
volume = {256},
year = {1982},
bdsk-url-1 = {http://dx.doi.org/10.1086/159908},
}
@article{mathis09,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2009A%26A...506..811M},
author = {{Mathis}, S.},
doi = {10.1051/0004-6361/200810544},
journal = {\aap},
keywords = {hydrodynamics, waves, turbulence, methods: analytical, stars: rotation, stars: evolution},
month = {nov},
pages = {811-828},
title = {{Transport by gravito-inertial waves in differentially rotating stellar radiation zones. I - Theoretical formulation}},
volume = {506},
year = {2009},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/200810544},
}
@article{khokhlov99,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1999ApJ...524L.107K},
author = {{Khokhlov}, A.~M. and {H{\"o}flich}, P.~A. and {Oran}, E.~S. and {Wheeler}, J.~C. and {Wang}, L. and {Chtchelkanova}, A.~Y.},
doi = {10.1086/312305},
eprint = {arXiv:astro-ph/9904419},
journal = {\apjl},
keywords = {GAMMA RAYS: BURSTS, ISM: JETS AND OUTFLOWS, STARS: PULSARS: GENERAL, STARS: SUPERNOVAE: GENERAL, STARS: SUPERNOVAE: INDIVIDUAL: ALPHANUMERIC: SN 1998BW},
month = {oct},
pages = {L107-L110},
title = {{Jet-induced Explosions of Core Collapse Supernovae}},
volume = {524},
year = {1999},
bdsk-url-1 = {http://dx.doi.org/10.1086/312305},
}
@article{heger00,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000ApJ...528..368H},
author = {{Heger}, A. and {Langer}, N. and {Woosley}, S.~E.},
doi = {10.1086/308158},
eprint = {arXiv:astro-ph/9904132},
journal = {\apj},
keywords = {HYDRODYNAMICS, METHODS: NUMERICAL, STARS EARLY-TYPE, STARS: EVOLUTION, STARS: INTERIORS, STARS ROTATION},
month = {jan},
pages = {368-396},
title = {{Presupernova Evolution of Rotating Massive Stars. I. Numerical Method and Evolution of the Internal Stellar Structure}},
volume = {528},
year = {2000},
bdsk-url-1 = {http://dx.doi.org/10.1086/308158},
}
@article{yoon05,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2005A%26A...443..643Y},
author = {{Yoon}, S.-C. and {Langer}, N.},
doi = {10.1051/0004-6361:20054030},
eprint = {arXiv:astro-ph/0508242},
journal = {\aap},
keywords = {stars: rotation, stars: evolution, stars: Wolf-Rayet, supernovae: general, gamma rays: bursts},
month = {nov},
pages = {643-648},
title = {{Evolution of rapidly rotating metal-poor massive stars towards gamma-ray bursts}},
volume = {443},
year = {2005},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20054030},
}
@article{jcd08,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2008Ap%26SS.316..113C},
archiveprefix = {arXiv},
author = {{Christensen-Dalsgaard}, J.},
doi = {10.1007/s10509-007-9689-z},
eprint = {0710.3106},
journal = {\apss},
keywords = {Stars: oscillations, Numerical methods, Asteroseismology},
month = {aug},
pages = {113-120},
title = {{ADIPLS{\mdash}the Aarhus adiabatic oscillation package}},
volume = {316},
year = {2008},
bdsk-url-1 = {http://dx.doi.org/10.1007/s10509-007-9689-z},
}
@article{2012A&A...548A..10M,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012A%26A...548A..10M},
archiveprefix = {arXiv},
author = {{Mosser}, B. and {Goupil}, M.~J. and {Belkacem}, K. and {Marques}, J.~P. and {Beck}, P.~G. and {Bloemen}, S. and {De Ridder}, J. and {Barban}, C. and {Deheuvels}, S. and {Elsworth}, Y. and {Hekker}, S. and {Kallinger}, T. and {Ouazzani}, R.~M. and {Pinsonneault}, M. and {Samadi}, R. and {Stello}, D. and {Garc{\'{\i}}a}, R.~A. and {Klaus}, T.~C. and {Li}, J. and {Mathur}, S. and {Morris}, R.~L.},
doi = {10.1051/0004-6361/201220106},
eid = {A10},
eprint = {1209.3336},
journal = {\aap},
keywords = {stars: oscillations, stars: interiors, stars: rotation, stars: late-type},
month = {dec},
pages = {A10, 14pp},
primaryclass = {astro-ph.SR},
title = {{Spin down of the core rotation in red giants}},
volume = {548},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201220106},
}
@article{2012A&A...540A.143M,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012A%26A...540A.143M},
archiveprefix = {arXiv},
author = {{Mosser}, B. and {Goupil}, M.~J. and {Belkacem}, K. and {Michel}, E. and {Stello}, D. and {Marques}, J.~P. and {Elsworth}, Y. and {Barban}, C. and {Beck}, P.~G. and {Bedding}, T.~R. and {De Ridder}, J. and {Garc{\'{\i}}a}, R.~A. and {Hekker}, S. and {Kallinger}, T. and {Samadi}, R. and {Stumpe}, M.~C. and {Barclay}, T. and {Burke}, C.~J.},
doi = {10.1051/0004-6361/201118519},
eid = {A143},
eprint = {1203.0689},
journal = {\aap},
keywords = {stars: oscillations, stars: interiors, stars: evolution, stars: late-type, methods: data analysis, asteroseismology},
month = {apr},
pages = {A143, 11pp},
primaryclass = {astro-ph.SR},
title = {{Probing the core structure and evolution of red giants using gravity-dominated mixed modes observed with Kepler}},
volume = {540},
year = {2012},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361/201118519},
}
@article{Shiode:2012,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2012arXiv1210.5525S},
archiveprefix = {arXiv},
author = {{Shiode}, J.~H. and {Quataert}, E. and {Cantiello}, M. and {Bildsten}, L.},
eprint = {1210.5525},
journal = {\arXiv:1210.5525},
keywords = {Astrophysics - Solar and Stellar Astrophysics},
month = {oct},
primaryclass = {astro-ph.SR},
title = {{The Observational Signatures of Convectively Excited Internal Gravity Modes in Main Sequence Stars}},
year = {2012},
}
@article{braithw06,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2006A%26A...450.1077B},
author = {{Braithwaite}, J. and {Nordlund}, {\AA}.},
doi = {10.1051/0004-6361:20041980},
eprint = {arXiv:astro-ph/0510316},
journal = {\aap},
keywords = {instabilities, magnetohydrodynamics (MHD), stars: magnetic fields},
month = {may},
pages = {1077-1095},
title = {{Stable magnetic fields in stellar interiors}},
volume = {450},
year = {2006},
bdsk-url-1 = {http://dx.doi.org/10.1051/0004-6361:20041980},
}
@book{hamming62,
author = {{Hamming}, R.~W.},
publisher = {McGraw-Hill, New York},
title = {{Numerical methods for scientists and engineers}},
year = {1962},
}
@article{ando86,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1986A%26A...163...97A},
author = {{Ando}, H.},
journal = {\aap},
keywords = {B STARS, STELLAR MASS EJECTION, STELLAR OSCILLATIONS, WAVE INTERACTION, FORMALISM, NONLINEAR EQUATIONS, ROTARY STABILITY, STELLAR MODELS},
month = {jul},
pages = {97-104},
title = {{Wave-rotation interaction and episodic mass-loss in Be stars}},
volume = {163},
year = {1986},
}
@article{ando85,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1985PASJ...37...47A},
author = {{Ando}, H.},
journal = {\pasj},
keywords = {ROTATION, STELLAR MODELS, STELLAR OSCILLATIONS, STELLAR ROTATION, WAVE INTERACTION, EXCITATION, INTEGRALS, KELVIN-HELMHOLTZ INSTABILITY, SOLAR OSCILLATIONS, VIBRATION MODE},
pages = {47-67},
title = {{Examination of wave behaviors in the differentially rotating systems}},
volume = {37},
year = {1985},
}
@article{ando83,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1983PASJ...35..343A},
author = {{Ando}, H.},
journal = {\pasj},
keywords = {REYNOLDS STRESS, STELLAR OSCILLATIONS, STELLAR ROTATION, WAVE PROPAGATION, ANGULAR MOMENTUM, BINARY STARS, ENERGY DISSIPATION, RADIATION TRAPPING, VARIABLE STARS, WAVE EXCITATION},
pages = {343-353},
title = {{Wave-rotation interaction in stars}},
volume = {35},
year = {1983},
}
@article{ando82,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1982A%26A...108....7A},
author = {{Ando}, H.},
journal = {\aap},
keywords = {ENERGY TRANSFER, KELVIN-HELMHOLTZ INSTABILITY, STELLAR ROTATION, WAVE EXCITATION, WAVE INTERACTION, ANGULAR MOMENTUM, CONVECTIVE FLOW, OSCILLATING FLOW, REYNOLDS STRESS, ROTATING BODIES, THERMODYNAMICS},
month = {apr},
pages = {7-13},
title = {{Active picture of rotation}},
volume = {108},
year = {1982},
}
@article{ando81,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1981MNRAS.197.1139A},
author = {{Ando}, H.},
journal = {\mnras},
keywords = {B STARS, KELVIN-HELMHOLTZ INSTABILITY, STELLAR ROTATION, VARIABLE STARS, BOUSSINESQ APPROXIMATION, FLOW EQUATIONS, MAGNETOHYDRODYNAMIC FLOW, PERIODIC VARIATIONS, STELLAR ENVELOPES, STELLAR EVOLUTION, STELLAR STRUCTURE},
month = {dec},
pages = {1139-1152},
title = {{Kelvin-Helmholtz instabilities and their application to B-type variables}},
volume = {197},
year = {1981},
}
@article{Maeder:1987,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/1987A%26A...173..247M},
author = {{Maeder}, A.},
journal = {\aap},
keywords = {ABUNDANCE, HERTZSPRUNG-RUSSELL DIAGRAM, STELLAR EVOLUTION, STELLAR MODELS, SURFACE REACTIONS, ASTRONOMICAL MAPS, O STARS, STELLAR MASS EJECTION, SUPERGIANT STARS, WOLF-RAYET STARS},
month = {feb},
pages = {247-262},
title = {{Changes of surface chemistry for standard massive star evolution - Cartography in the HR diagram}},
volume = {173},
year = {1987},
}
@book{Quataert_2005,
title = {{The evolution of AGB stars with convective overshoot}},
isbn = {9780511818868},
url = {http://dx.doi.org/10.1017/CBO9780511818868.014},
doi = {10.1017/CBO9780511818868.014},
number = {2},
publisher = {Cambridge University Press},
author = {{Herwig}, F.},
year = {2000},
pages = {952-968},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...360..952H},
eprint = {arXiv:astro-ph/0007139},
journal = {\aap},
keywords = {STARS: ABUNDANCES, STARS: INTERIORS, STARS: EVOLUTION, STARS: AGB AND POST-AGB},
month = {aug},
volume = {360},
}
@ARTICLE{2012ApJ...753...22B,
author = {{Brown}, P.~J. and {Dawson}, K.~S. and {de Pasquale}, M. and {Gronwall}, C. and {Holland}, S. and {Immler}, S. and {Kuin}, P. and {Mazzali}, P. and {Milne}, P. and {Oates}, S. and {Siegel}, M.},
title = {{A Swift Look at SN 2011fe: The Earliest Ultraviolet Observations of a Type Ia Supernova}},
journal = {\apj},
archiveprefix = {arXiv},
eprint = {1110.2538},
primaryclass = {astro-ph.CO},
keywords = {galaxies: distances and redshifts, supernovae: general, ultraviolet: general},
year = {2012},
month = {jul},
volume = {753},
eid = {22},
pages = {22},
doi = {10.1088/0004-637X/753/1/22},
adsurl = {http://adsabs.harvard.edu/abs/2012ApJ...753...22B},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
}
@article{herwig_2000_aa,
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...360..952H},
author = {{Herwig}, F.},
eprint = {arXiv:astro-ph/0007139},
journal = {\aap},
keywords = {STARS: ABUNDANCES, STARS: INTERIORS, STARS: EVOLUTION, STARS: AGB AND POST-AGB},
month = {aug},
pages = {952-968},
title = {{The evolution of AGB stars with convective overshoot}},
volume = {360},
year = {2000},
}
@book{Brown_2012,
title = {{The evolution of AGB stars with convective overshoot}},
url = {http://dx.doi.org/10.4271/2012-01-1850},
doi = {10.4271/2012-01-1850},
number = {0},
institution = {SAE International},
author = {{Herwig}, F.},
year = {2000},
month = {aug},
adsnote = {Provided by the SAO/NASA Astrophysics Data System},
adsurl = {http://adsabs.harvard.edu/abs/2000A%26A...360..952H},
eprint = {arXiv:astro-ph/0007139},
journal = {\aap},
keywords = {STARS: ABUNDANCES, STARS: INTERIORS, STARS: EVOLUTION, STARS: AGB AND POST-AGB},
pages = {952-968},
volume = {360},
}
@article{Cantiello_1997,
volume = {17},
url = {http://dx.doi.org/10.1023/A:1027381412574},
doi = {10.1023/A:1027381412574},
number = {2},
journal = {Bioscience Reports},
publisher = {Portland Press},
author = {Cantiello, Horacio F.},
year = {1997},
pages = {147-171},
}
