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The Various Scenarios Leading to WR Stars: Their Relative Importance and the Role of Mixing

Published online by Cambridge University Press:  14 August 2015

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

Extract

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Over the last 40 years WR stars have been associated with almost all possible evolutionary stages. Hereafter are listed those scenarios which may be considered as most relevant in view of recent surface abundance determinations (cf. Willis, this meeting).

Type
SESSION 5 — EVOLUTIONARY STATUS OF WOLF-RAYET STARS
Copyright
Copyright © Reidel 1982 

References

Appenzeller, I. 1970, Astron. Astrophys. 5, 355; 9, 216.Google Scholar
Azzopardi, M., Breysacher, J. 1979, Astron. Astrophys. 75, 120.Google Scholar
Breysacher, J. 1981, Astron. Astrophys. Suppl. 43, 203.Google Scholar
Conti, P.S. 1975, Mém. Soc. Roy. Sci. Liège IX, p. 193.Google Scholar
De Loore, C. 1980, Review in IAU Colloquium 59, Effects of Mass Loss in Stellar Evolution, in press.CrossRefGoogle Scholar
Kippenhahn, R., Thomas, H.C. 1981, IAU Symposium 93, p. 237.Google Scholar
Lequeux, J. 1979, Astron. Astrophys. 80, 35.Google Scholar
Maeder, A. 1976, Astron. Astrophys. 47, 389.Google Scholar
Maeder, A. 1980, Astron. Astrophys. 92, 101.Google Scholar
Maeder, A. 1981a, Astron. Astrophys. 99, 97; 1981b, c, in press.Google Scholar
Noels, A., Gabriel, M. 1981, Astron. Astrophys. 101, 215.Google Scholar
Schatzman, E. 1977, Astron. Astrophys. 56, 211.Google Scholar
Schatzman, E., Maeder, A. 1981, Astron. Astrophys. 96, 1.Google Scholar
Vanbeveren, D., Conti, P.S. 1980, Astron. Astrophys. 88, 230.Google Scholar
Van der Hucht, K.A., Conti, P.S., Lundström, I., Stenholm, B. 1981, Sp. Sc. Rev. 28, 227.CrossRefGoogle Scholar
Zahn, J.P. 1974, IAU Symposium 59, p. 185.Google Scholar