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On the evolutionary time scale of the accreting component in massive close binaries: consequences for the supernova event

Published online by Cambridge University Press:  12 April 2016

C. Doom  and
J.P. De Grève
C. Doom
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel
J.P. De Grève
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel

Abstract

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The remaining core hydrogen burning lifetime after a case B of mass exchange is computed for the mass gaining component in massive close binaries. Effects of stellar wind mass loss and mass loss during Roche Lobe OverFlow (RLOF) are included. Consequences for the evolutionary scenario are discussed.

Type
Session VIII - Effects of Mass Loss on the Evolution of Binary Stars
Information
International Astronomical Union Colloquium , Volume 59: Effects of Mass Loss on Stellar Evolution , 1981 , pp. 465 - 468
Copyright
Copyright © Reidel 1981

References

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