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Stellar evolution including diffusion and matter flow induced by mass-loss

Published online by Cambridge University Press:  19 December 2013

O. Richard  and
M. Vick
O. Richard
Affiliation:
LUPM, Université Montpellier II, CNRS, cc072, Place E. Bataillon, 34095 Montpellier Cedex, France
M. Vick
Affiliation:
LUPM, Université Montpellier II, CNRS, cc072, Place E. Bataillon, 34095 Montpellier Cedex, France Département de Physique, Université de Montréal, Montréal, Québec, H3C 3J7, Canada
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Abstract

It is clear that in order to explain many observed stellar phenomenae, atomic diffusion must be included in stellar models. Observed surface abundances allow us to constrain other transport pro- cesses which compete with atomic diffusion. We will focus on the effect of the flow of matter induced by mass-loss in stellar models.

Type
Research Article
Information
European Astronomical Society Publications Series , Volume 63: New Advances in Stellar Physics: From Microscopic to Macroscopic Processes , 2013 , pp. 349 - 356
Copyright
© EAS, EDP Sciences, 2013

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