Initial masses of stars changing into Wolf-Rayet stars

Details Initial masses of stars changing into Wolf-Rayet stars Initial masses of stars changing into Wolf-Rayet stars

Jun 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985azh....62..604t&link_type=abstract

(Astronomicheskii Zhurnal, vol. 62, May-June 1985, p. 604, 605) Soviet Astronomy (ISSN 0038-5301), vol. 29, May-June 1985, p. 35

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Star Distribution, Stellar Evolution, Stellar Mass, Supermassive Stars, Wolf-Rayet Stars, B Stars, O Stars

Scientific paper

The structural characteristics of Wolf-Rayet stars are considered. It is shown that the spatial distribution and ratio of populations in O-type and B-type Wolf-Rayet stars are consistent with the hypothesis that components of close binary systems (masses less than about 20 solar mass) become Wolf-Rayet stars. All other stars with masses greater than about 40 solar mass also become Wolf-Rayet stars.

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