The evolution of the mass gainer in massive close binaries.

Astronomy and Astrophysics – Astrophysics

Scientific paper

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Binaries: Close, Stars: Evolution, X-Rays: Stars

Scientific paper

In this paper we critically discuss the physics and the behaviour of a star which is subjected to a large mass gain process as is the case during the Roche lobe overflow in a close binary. Arguments are given in favor of large scale mixing of the star during accretion. Evolutionary computations are presented where this large scale mixing process is included; the results are compared to classsical accretion models.

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