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Radial and Non-Radial Pulsations in Wolf-Rayet Stars and in Supergiants

Published online by Cambridge University Press:  30 March 2016

André Maeder
André Maeder*
Affiliation:
Geneva Observatory, CH-1290 Sauverny, Switzerland

Extract

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The two subjects of the variability of WR stars and of supergiants are still in their infancy and are certainly promised to a great development in coming years. The physics and pulsation properties of WR stars and supergiants, although both kinds of stars result from massive star evolution, are indeed very different and will be discussed separately.

Type
Joint Discussions
Information
Highlights of Astronomy , Volume 7: Highlights of Astronomy. As presented at the XIXth General Assembly of the IAU, 1985 , 1986 , pp. 273 - 281
Copyright
Copyright © Reidel 1986

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