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Evolution of Massive Stars with Rotation and Mass Loss

Published online by Cambridge University Press:  26 May 2016

André Maeder  and
Georges Meynet
André Maeder
Affiliation:
Geneva Observatory, CH–1290 Sauverny, Switzerland
Georges Meynet
Affiliation:
Geneva Observatory, CH–1290 Sauverny, Switzerland

Abstract

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Rotation appears as a dominant effect in massive star evolution. It largely affects all the model outputs: inner structure, tracks, lifetimes, isochrones, surface compositions, blue to red supergiant ratios, etc. At lower metallicities, the effects of rotational mixing are larger; also, more stars may reach critical velocity, even if the initial distribution of rotational velocities is the same.

Type
Session 4 Rotation and Stellar Evolution
Information
Symposium - International Astronomical Union , Volume 215: Stellar Rotation , 2004 , pp. 500 - 509
Copyright
Copyright © Astronomical Society of the Pacific 2004 

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