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Non conservative massive binary evolution (how much mass leaves the bnary during the evolution from OB+OB to WR+OB)

Published online by Cambridge University Press:  12 April 2016

D. Vanbeveren
D. Vanbeveren*
Affiliation:
Astrophysical Institute, Vrije Universiteit Brussel, Belgium

Extract

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The observations give us on one hand the mass ratio (q) distribution of OB+OB type binaries in a stage prior to Roche lobe overflow (RLOF), and on the other hand the q distribution of WR binaries which are considered to be in a stage after RLOF. By comparing both distributions one may hope to be able to say something about the mass loss during RLOF.

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. 461 - 463
Copyright
Copyright © Reidel 1981