How we can learn from studies of wide binary statistics

Details How we can learn from studies of wide binary statistics How we can learn from studies of wide binary statistics

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142..277w&link_type=abstract

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

Astronomy and Astrophysics

Astrophysics

6

Binary Stars, Star Distribution, Statistical Distributions, Stellar Models, Astronomical Catalogs, Density (Number/Volume)

Scientific paper

The author presents a versatile technique for comparing wide binary observations with theoretical semi-major axis distributions. To illustrate this technique, the theoretical implications of the recent Latham et al. (1984) data on wide binaries are examined. Motivated by the apparent high number density of wide binaries implied by the Latham et al. sample, the author defines a criterion for selecting candidate wide binaries form the Yale Bright Star Catalog. The candidate list is used to determine an upper bound for wide binary density of nWB = 4×10-3pc-3.

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