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The effect of turbulent mixing on the g-mode spectrum of MS stars

✍ Scribed by J. Montalbán; A. Miglio; P. Eggenberger; A. Noels

Publisher
John Wiley and Sons
Year
2008
Tongue
English
Weight
563 KB
Volume
329
Category
Article
ISSN
0004-6337

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✦ Synopsis

Abstract

Understanding transport processes inside stars is one of the main goals of asteroseismology. Chemical turbulent mixing can affect the internal distribution of μ near the energy generating core, having an effect on the evolutionary tracks similar to that of overshooting. This mixing leads to a smoother chemical composition profile near the edge of the convective core, which is reflected in the behavior of the buoyancy frequency and, therefore, in the frequencies of gravity modes. We describe the effects of convective overshooting and turbulent mixing on the frequencies of gravity modes in B‐type main sequence stars. In particular, the cases of p‐g mixed modes in β Cep stars and high‐order modes in SPBs are considered. (© 2008 WILEY‐VCH Verlag GmbH & Co. KGaA, Weinheim)

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