The combined effect of mass loss and overshooting. III Evolutionary scenarios for massive close binaries

Details The combined effect of mass loss and overshooting. III Evolutionary scenarios for massive close binaries The combined effect of mass loss and overshooting. III Evolutionary scenarios for massive close binaries

Apr 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983a%26a...120...97d&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 120, no. 1, April 1983, p. 97-105. Sponsorship: Fonds de la Recherche Fondamen

Astronomy and Astrophysics

Astrophysics

31

Binary Stars, Stellar Evolution, Stellar Mass Accretion, Stellar Mass Ejection, Wolf-Rayet Stars, X Ray Sources, O Stars, Stellar Models, X Ray Binaries

Scientific paper

The evolution of massive close binaries is revised by taking into account overshooting from convective cores. Nine different evolutionary scenarios are presented, resulting from the introduction of an Of phase for each component. The theoretical results are compared to observations of Wolf-Rayet binaries and X-ray binaries. It is found that X-ray binaries originate from the lower mass Wolf-Rayet binaries. The existence of WR+Of stars is predicted.

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