AUTHOREA
Log in
Sign Up
Browse Preprints
LOG IN
SIGN UP
this is for holding javascript data
Sub-surface convection zones in hot massive stars and their observable consequences
/
layout.md
Abstract.tex Introduction.tex method.tex Eq: Diffusion Equation.tex MLT.tex Eq: Ledoux Criterion.tex Eq: Ficks Law.tex Eq: Diffusion Convection.tex Winds and Composition.tex figures/varkappa/opacity.png Helium Convection Zone.tex Eq: Rayleigh Criterion.tex Development of Convection.tex Results.tex figures/20zsunsurf/subsurface1.png figures/60zsunsurf/subsurface2.png As_outlined_above.tex Eq: Average.tex The_radial_extent_of.tex clumps.tex From_Figuresref20zsunsurf_andref60zsunsurf_three.tex While_in_the_discussed.tex Grid.tex itemize_item_For_given_luminosity.tex subsectionRotating_modelslabelrotation_We_considered.tex As_pointed_out_by.tex figures/feczrotating/velocity.png sectionComparison_with_observationslabelcomparison.tex In_the_following_we.tex subsectionMicroturbulencelabelmicro.tex The_convective_cells_in.tex Eq: Acoustic Waves Flux.tex Eq: Gravity Waves Flux.tex resulting_in_maximum_emission.tex The_BruntVaisala_frequency_in.tex Eq: Energy Ratio.tex Eq: Velocity.tex Again_multidimensional_hydrodynamic_simulations.tex figures/sketch/sketch.png equation_Deltalambda_D__fraclambdacsqrtfrac2_mathcalR.tex The_microturbulent_velocity.tex Photospheric_microturbulence_is_routinely.tex figures/vsinimicro/rotational_velocity.png In_Figrefmicrolmc_we_show.tex figures/microlmc/micro1.png In_order_to_compare.tex figures/grwplot/energy.png Figurerefhrdvel_shows_the_isocontours.tex figures/hrdvel/microturbulence.png Significant Correlation.tex A Physical Origin of Microturbulence.tex Mass Discrepancy.tex figures/discrepancy/discrepancy.png Nonradial Pulsations.tex Several_classes_of_OBstar.tex Connections to Observations.tex Observationally_the_classical_betaCephei.tex Pulsation and Microturbulence.tex Comparing_Figrefpulsationplot_with_the.tex figures/pulsationplot/pulsation.png Wind Clumping.tex Clumps Size.tex Clumping in WR.tex Clumping in O Stars.tex Line Driven Instability.tex Clumping and Subsurface Convection.tex figures/clumpvel/clumping.png Estimate Clumps Number.tex Line Profile Variability.tex subsectionMagnetic_fieldslabelmagnetic.tex Eq: Equipartition.tex Buoyant Rise.tex As_a_consequence_even.tex Rotation_may_play_an.tex Surface Magnetic Fields.tex Connection With Surface Phenomena.tex More Implications.tex sectionConcluding_remarks.tex Hot_luminous_stars_show.tex Microturbulence.tex In_Sectrefmagnetic_we_proposed.tex The_FeCZ_could_also.tex Finally_we_note_that.tex Acknowledgements.tex