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Massive Star Evolution
Published online by Cambridge University Press: 25 May 2016
Abstract
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
References
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