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Conservative and non-conservative evolutionary computations in connection with Wolf-Rayet binaries.

Published online by Cambridge University Press:  14 August 2015

D. Vanbeveren ,
J.P. De Grève ,
C. de Loore  and
E.L. van Dessel
D. Vanbeveren
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel
J.P. De Grève
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel
C. de Loore
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel
E.L. van Dessel
Affiliation:
Royal Belgian Observatory

Extract

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We consider the evolution of massive close binaries. The reader is referred to the first contribution by the same authors during this conference for the general ideas. The present contribution deals with the implications for the Wolf-Rayet phase, i.e. that part of the evolution where the primary is liable to show W-R characteristics (as usual the primary is defined as the originally more massive component). We refer to the evolution after the exchange of mass between the components, or even during the exchange phase (see section 3).

Type
Session 8: Evolutionary Scenario and the WR Connection
Information
Symposium - International Astronomical Union , Volume 83: Mass Loss and Evolution of O-Type Stars , 1979 , pp. 483 - 488
Copyright
Copyright © Reidel 1979 

References

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