The distribution of detached main-sequence type close binary systems with respect to masses and component mass ratios

Details The distribution of detached main-sequence type close binary systems with respect to masses and component mass ratios The distribution of detached main-sequence type close binary systems with respect to masses and component mass ratios

Aug 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989azh....66..790k&link_type=abstract

Astronomicheskii Zhurnal (ISSN 0004-6299), vol. 66, July-Aug. 1989, p. 790-800. In Russian.

Astronomy and Astrophysics

Astronomy

2

Binary Stars, Main Sequence Stars, Stellar Mass, Astronomical Photometry, Mass Distribution, Mass Ratios, Star Formation, Tables (Data)

Scientific paper

Close binary systems with both components in the luminosity class V are studied, taking into account the geometric and photometric effects of observational selection. The current mass distributions of both components have been obtained and the star formation function has been estimated. The star formation function can be represented by a power law that is similar to the star formation function for the primary components of close binary systems obtained by Karicheva et al. (1978).

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