The theoretical expected galactic distribution of WR runaway stars

Details The theoretical expected galactic distribution of WR runaway stars The theoretical expected galactic distribution of WR runaway stars

Sep 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982a%26a...113..205v&link_type=abstract

Astronomy and Astrophysics, vol. 113, no. 2, Sept. 1982, p. 205-210.

Astronomy and Astrophysics

Astrophysics

B Stars, Binary Stars, Galactic Structure, O Stars, Stellar Evolution, Wolf-Rayet Stars, Stellar Mass, Supernovae, Tables (Data)

Scientific paper

A statistical study is presented on the theoretical expected number of WR + OB binaries, WR + compact star systems, WR single runaway stars and normal WR single stars. Starting from a complete sample of O type single stars and close binaries, imposing a mass ratio distribution for the binaries and an initial mass function for single stars and primaries of close binaries, evolution of massive stars is used to determine the theoretical expected absolute average distance difference of the WR runaways and of the single lined WR stars in general, relative to the birthplace of their progenitor OB type stars.

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