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Deep inside low-mass stars

Published online by Cambridge University Press:  01 April 2008

Corinne Charbonnel  and
Suzanne Talon
Corinne Charbonnel
Affiliation:
Geneva Observatory, University of Geneva, ch. des Maillettes 51, 1290 Versoix, Switzerland email: [email protected] Laboratoire d'Astrophysique de Toulouse-Tarbes, Université de Toulouse, CNRS UMR 5572, 14 Av. E.Belin, 31400 Toulouse, France
Suzanne Talon
Affiliation:
RQCHP, Département de physique, Université de Montréal, C. P. 6128, succ. centre-ville, Montréal, Québec, H3C 3J7 email: [email protected]
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Abstract

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Low-mass stars exhibit, at all stages of their evolution, the signatures of complex physical processes that require challenging modeling beyond standard stellar theory. In this review, we recall the most striking observational evidences that probe the interaction and interdependence of various transport processes of chemicals and angular momentum in these objects. We then focus on the impact of atomic diffusion, large scale mixing due to rotation, and internal gravity waves on stellar properties on the main sequence and slightly beyond.

Keywords

hydrodynamics - instabilities - turbulence - waves - stars: abundances- stars: evolution - stars: interiors - stars: rotation
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 4 , Symposium S252: The Art of Modeling Stars in the 21st Century , April 2008 , pp. 163 - 174
Copyright
Copyright © International Astronomical Union 2008

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