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Small and Intermediate Mass Stellar Evolution - Main Sequence and Close to It

Published online by Cambridge University Press:  12 April 2016

A. Noels  and
N. Grevesse
A. Noels
Affiliation:
Institut d’Astrophysique Université de Liège, 5, avenue de Cointe, B-4000LIEGE-BELGIUM
N. Grevesse
Affiliation:
Institut d’Astrophysique Université de Liège, 5, avenue de Cointe, B-4000LIEGE-BELGIUM

Abstract

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We present the standard models for small and intermediate main sequence stars and we discuss some of the problems arising with semiconvection and overshooting. The surface abundance of Li serves as a test for other physical mechanisms, including microscopic and turbulent diffusion, rotation and mass loss.

Type
V. The changing interior
Information
International Astronomical Union Colloquium , Volume 137: Inside the Stars , 1993 , pp. 410 - 425
Copyright
Copyright © Astronomical Society of the Pacific 1993

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