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Massive Star Evolution

Published online by Cambridge University Press:  25 May 2016

N. Langer  and
A. Heger
N. Langer
Affiliation:
Institut für Physik, Universität Potsdam Postfach 601553, D-14415 Potsdam, Germany
A. Heger*
Affiliation:
Max-Planck-Institut für Astrophysik Postfach 1523, D-85740 Garching, Germany
*
1present address: UCO/Lick Observatory, UC Santa Cruz, CA 95064, USA

Abstract

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The evolution of massive stars is far from being fully understood, as we outline by pointing to a number of open problems related to massive stars in the Magellanic Clouds. We argue that rotation may be a key ingredient in the physics of massive stars. We report on recent results obtained including rotation, and their relevance to these remaining questions.

Type
Part 3. Massive Stars and 30 Doradus
Information
Symposium - International Astronomical Union , Volume 190: New Views of the Magellanic Clouds , 1999 , pp. 192 - 199
Copyright
Copyright © Astronomical Society of the Pacific 1999 

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