The evolution of massive close binaries revised

Details The evolution of massive close binaries revised The evolution of massive close binaries revised

Dec 1991

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1991a%26a...252..159v&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 252, no. 1, Dec. 1991, p. 159-171.

Astronomy and Astrophysics

Astrophysics

54

Binary Stars, Massive Stars, Nuclear Astrophysics, Stellar Evolution, Mass To Light Ratios, Stellar Winds, Wolf-Rayet Stars

Scientific paper

Evolution computations of massive close binaries are presented using
improved stellar wind mass loss rate formalisms during core hydrogen and
core helium burning, improved physics and mass loss rates during the
luminous blue variable phase of the most massive stars. The computations
are compared with recent observations of WR stars.

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