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1993•International Astronomical Union ColloquiumOpen access

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

A. Noels, N. Grevesse

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Abstract

Abstract 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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Abstract 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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Available abstract

Abstract 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.

Key concepts: Main sequence, Sequence (biology), Stars, Physics, Diffusion, Astrophysics, Rotation (mathematics), Stellar evolution

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