Stellar models for a wide range of initial chemical compositions until helium burning

• 15 November 1997
• journal article
• Published by EDP Sciences in Astronomy and Astrophysics Supplement Series
• Vol. 125  (3) , 439-443
• https://doi.org/10.1051/aas:1997378

Abstract

Keywords

• EVOLUTION
• NUCLEAR REACTIONS
• MOMENT OF INERTIA
• RADIUS OF GYRATION
• MAIN SEQUENCE
• SPIN ORBIT COUPLING
• BINARY STAR
• CHEMICAL COMPOSITION
• COMPARATIVE STUDY