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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
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
Vanbeveren, D., De Grève, J.P., van Desse, E.L.,de Loore, C.:1979, Astron.Astrophys.
73,19.Google Scholar