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The role of rotation in the evolution of massive stars losing mass

Published online by Cambridge University Press:  14 August 2015

S. R. Sreenivasan  and
W.J.F. Wilson
S. R. Sreenivasan
Affiliation:
Department of Physics, The University of Calgary, Calgary, Alberta, Canada T2N 1N4
W.J.F. Wilson
Affiliation:
Department of Physics, The University of Calgary, Calgary, Alberta, Canada T2N 1N4

Abstract

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The role of differential and solid body rotation in the evolution of massive stars undergoing mass loss is discussed. The implications for Of, WR, β Cephei stars and shell stars are brought out.

Type
Session 6: Evolution with Mass Loss: Single Stars
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 367 - 370
Copyright
Copyright © Reidel 1979 

References

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De Loore, C.: (1978) Review paper on Mass loss from Single Stars (this volume).Google Scholar
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Snow, T.P.: (1978) Review paper on Mass loss observations (this volume).Google Scholar
Sreenivasan, S.R. and Wilson, W.J.F.: 1978a, Astron. Astrophys. (in press).Google Scholar
Sreenivasan, S.R. and Wilson, W.J.F.: 1978b, Bull. AAS 10, 438.Google Scholar
Sreenivasan, S.R. and Wilson, W.J.F.: 1978c, Proc. Conf. Stellar Pulsational Instabilities, Greenbelt, MD (in press).Google Scholar