Small and intermediate mass stellar evolution - Main sequence and close to it

Details Small and intermediate mass stellar evolution - Main sequence and close to it Small and intermediate mass stellar evolution - Main sequence and close to it

Jan 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993aspc...40..410n&link_type=abstract

In: Inside the stars; Proceedings of the 137th IAU Colloquium, Univ. of Vienna, Austria, Apr. 13-18, 1992 (A93-53126 23-90), p.

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5

Main Sequence Stars, Stellar Evolution, Stellar Mass, Stellar Models, Abundance, Computational Astrophysics, Lithium, Star Clusters, Stellar Convection, Stellar Mass Ejection, Stellar Rotation

Scientific paper

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.

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