Evolution of massive binaries including the effect of convective core overshooting

Details Evolution of massive binaries including the effect of convective core overshooting Evolution of massive binaries including the effect of convective core overshooting

Oct 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...224...93v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 224, no. 1-2, Oct. 1989, p. 93-97.

Astronomy and Astrophysics

Astrophysics

10

Binary Stars, Convection Currents, Stellar Evolution, Stellar Mass, Stellar Spectra, B Stars, O Stars, Stellar Mass Accretion, Stellar Mass Ejection, Wolf-Rayet Stars

Scientific paper

Calculations are presented for the evolution of massive close binaries with initial periods larger than 3 days, including the effect of convective core overshooting during core H burning (Maeder and Meynet, 1987). The evolution of the mass gainer during the Roche lobe overflow phase of the mass loser is examined. The results are compared with observations of WR + OB binaries, suggesting that mass transfer during the Roche lobe overflow phase of the mass loser plays a fundamental role in binary formation.

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