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Models of rotating Wolf-Rayet stars

Published online by Cambridge University Press:  07 August 2017

J. Fliegner  and
N. Langer
J. Fliegner
Affiliation:
MPI für Astrophysik, D-85740 Garching, B.R. Deutschland
N. Langer
Affiliation:
MPI für Astrophysik, D-85740 Garching, B.R. Deutschland

Abstract

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We explore the influence of rotation on the evolution of massive stars (40 M⊙). We find the evolution in the HRD, the initial-final mass relation, and the duration of the various WR phases to depend sensitively on the initial rotation rate. We predict that, independent of the initial rotation rate, the majority of WR stars should be slow rotators.

Type
Session V - poster summaries
Information
Symposium - International Astronomical Union , Volume 163: Wolf-Rayet Stars: Binaries, Colliding Winds, Evolution , 1995 , pp. 326 - 328
Copyright
Copyright © Kluwer 1995 

References

Endal, A.S., Sofia, S. 1978, ApJ 220, 279 CrossRefGoogle Scholar
Langer, N., Hamann, W.-R., Lennon, M., Najarro, F., Pauldrach, A.W.A., Puls, J. 1994, A&A , in press Google Scholar
Maeder, A. 1987, A&A 178, 159 Google Scholar
Maheswaran, M., Cassinelli, J.P. 1994, in press Google Scholar
Pinsonneault, M.H., Kawaler, S.D., Sofia, S., Demarque, D. 1989, ApJ 338, 424 Google Scholar