Matteo Cantiello edited abstract.tex  almost 9 years ago

Commit id: 52f4dadeb06c4590762a2ec47cc587a517cc572c

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core, in over 3500 red giant stars. About 20\% of our sample have mode  suppression but this fraction is a strong function of mass. Strong core fields occur only in stars above 1.1 solar masses,  %[this setence seems to break flow between previous and subsequent sentence] Low-mass red giants, which burned hydrogen in a radiative core, do not posses strong internal magnetic fields.   and for intermediate-mass stars (1.6--2.0 \msun), the occurence occurrence  is at least 60\%, suggesting that powerful dynamos are very common in the  convective cores of these stars.