Physics
Scientific paper
Jun 1983
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983nssl.conf..299b&link_type=abstract
The Nearby Stars and the Stellar Luminosity Function, Proceedings of IAU Colloquium No. 76 held 13-16 June 1983 at Wesleyan Univ
Physics
2
Scientific paper
Wide moving pair candidates have been identified in two samples of F, G and K dwarfs with ≡20 pc of the Sun. The results agree with previous examinations of the motions of A stars and K and M dwarf star samples, in that the apparent incidence of widely separated comoving stars in pairs greatly exceeds that which would be expected due to coincidental similarities of space motions.
Beavers Willet I.
Russell James L.
Simonson G. F.
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