Evolutionary sequences for massive close binaries with galactic abundances with Rogers-Iglesias opacities

Details Evolutionary sequences for massive close binaries with galactic abundances with Rogers-Iglesias opacities Evolutionary sequences for massive close binaries with galactic abundances with Rogers-Iglesias opacities

May 1994

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1994a%26as..105...21d&link_type=abstract

Astronomy and Astrophysics Suppl. 105, 21-28 (1994)

Astronomy and Astrophysics

Astrophysics

13

Binaries: Close, Stars: Mass-Loss, Stars: Evolution, Stars: Wolf-Rayet

Scientific paper

Evolutionary sequences for massive close binaries with (X,Z) = (0.7, 0.02) in the primary mass range 9 to 40 Msun_ and mass ratios 0.6 and 0.9 are presented. These computations were performed with the same program, with the same updated physics and opacity data as in the paper De Loore & Vanbeveren (1993) and form together with the results in the latter paper a complete set of simultaneous massive close binary evolutionary computations for the Galaxy and the Magellanic Clouds. A full discussion of these computations will be presented in a forthcoming paper (De Loore & Vanbeveren 1994).

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