Mass transfer in massive close binaries - The influence of the initial period

Details Mass transfer in massive close binaries - The influence of the initial period Mass transfer in massive close binaries - The influence of the initial period

Aug 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988a%26as...74..325d&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 74, no. 2, Aug. 1988, p. 325-329.

Astronomy and Astrophysics

Astrophysics

5

Binary Stars, Mass Transfer, Periodic Variations, Stellar Evolution, Wolf-Rayet Stars, Stellar Mass, Stellar Models, Stellar Orbits

Scientific paper

Models of the mass-losing component in massive mass transferring binaries evolving through a case AB of mass transfer are presented for three sets of masses and various initial periods. From the authors' results and similar ones published in the literature, relations are derived between the initial parameters and the parameters at the end of mass transfer for the mass range 20 to 30 M_sun;.

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