A photometric study of wide visual double stars. IV - UVBY photometry of wide visual double stars with G-type primaries

Details A photometric study of wide visual double stars. IV - UVBY photometry of wide visual double stars with G-type primaries A photometric study of wide visual double stars. IV - UVBY photometry of wide visual double stars with G-type primaries

Apr 1993

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1993a%26as...98...17s&link_type=abstract

Astronomy and Astrophysics Supplement Series (ISSN 0365-0138), vol. 98, no. 1, p. 17-20.

Astronomy and Astrophysics

Astrophysics

2

Double Stars, G Stars, Stellar Magnitude, Stellar Spectrophotometry, Stellar Temperature, Telescopes, Visual Photometry

Scientific paper

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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