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Mass-Loss From Spinning Stars

Published online by Cambridge University Press:  30 March 2016

S. R. Sreenivasan
S. R. Sreenivasan*
Affiliation:
Department of Physics, The University of Calgary, Calgary, Alberta, Canada

Abstract

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The effects of mass-loss and angular momentum loss on the evolution of massive stars are discussed bringing out the main results as well as the limitations of recent studies. It is pointed out that an acceptable theory of stellar winds in early as well as late type stars is needed as well as a satisfactory assessment of a number of instabilities in these contexts for an adequate understanding of the evolutionary consequences for a wide variety of population I and polulation II stars, which are affected by mass-loss.

Type
Joint Discussion
Information
Highlights of Astronomy , Volume 5: Highlights of Astronomy. As presented at the XVIIth General Assembly of the IAU, 1979 , 1980 , pp. 601 - 613
Copyright
Copyright © Cambridge University Press 1980

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