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A PHOTOMETRIC-STUDY OF WIDE VISUAL DOUBLE STARS .4. UVBY PHOTOMETRY OF WIDE VISUAL DOUBLE STARS WITH G-TYPE PRIMARIES

D SINACHOPOULOS,E VANDESSEL

Astronomy & Astrophysics Supplement Series（1993）

Cited 23|Views2
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Abstract
We performed uvby aperture photometry of wide visual double stars with G-type primaries. The minimum angular separation of the components is 10 arcsecs and mainly less than 20 arcsecs. As both components have often similar photometric and astrophysical parameters, we infer that most of these double stars have components of common origin.
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Key words
STARS, BINARIES, VISUAL,PHOTOMETRY
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