Statistical study of visual binaries

Details Statistical study of visual binaries Statistical study of visual binaries

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142..245v&link_type=abstract

(IAU, Colloquium on Wide Components in Double and Multiple Stars, 97th, Brussels, Belgium, June 8-13, 1987) Astrophysics and Spa

Physics

19

Binary Stars, Statistical Analysis, Stellar Physics, Visible Spectrum, Mass To Light Ratios, Star Distribution

Scientific paper

A statistical study of physical pairs from the IDS catalog has been
performed. For 2811 binaries with luminosity class V primaries, it has
been found that the mass function is a Salpeter one; their distribution
over semimajor axes of orbits is dN proportional to d log a. The rate of
duplicity of stars is close to 1.

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