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Chemical evolution and mixing processes in massive stars

Published online by Cambridge University Press:  07 August 2017

Knut Jørgen Røed Ødegaard
Knut Jørgen Røed Ødegaard*
Affiliation:
Institute of Theoretical Astrophysics University of Oslo, P.O. Box 1029 Blindern, N-0315 Oslo, Norway

Abstract

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The first results of new evolutionary calculations of massive stars are presented. The calculations cover ZAMS masses from 20—200 M⊙. Yields and abundances throughout the stars are presented.

Keywords

stars: massive starsevolutionnucleosynthesismixing

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