Visual binary systems in the solar neighbourhood - A question of their separations

Details Visual binary systems in the solar neighbourhood - A question of their separations Visual binary systems in the solar neighbourhood - A question of their separations

Nov 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989ap%26ss.161..241g&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 161, no. 2, Nov. 1989, p. 241-246.

Astronomy and Astrophysics

Astrophysics

Binary Stars, Early Stars, Late Stars, Main Sequence Stars, Solar Neighborhood, Statistical Analysis, Stellar Evolution, Stellar Luminosity, Stellar Spectra

Scientific paper

The separations between the components of nearby visual binaries are investigated. For Main-Sequence stars in the spectral range F0-M7 the distribution of the separations is independent from the spectral type of the primary component. A decrease of the limiting upper separation from the early to late-type systems found by Abt is probably due to selective constraints.

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