Photoelectric observations of CPM stars in the BVRI system

Details Photoelectric observations of CPM stars in the BVRI system Photoelectric observations of CPM stars in the BVRI system

Mar 1988

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1988ap%26ss.142..123r&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

2

Binary Stars, Magnetic Stars, Peculiar Stars, Stellar Spectrophotometry, Stellar Systems, Visible Spectrum, Companion Stars, Electrophotometry, Stellar Motions

Scientific paper

A photometric program to estimate the frequency of close unresolved companions in visual binary sytems has been developed. The sensitivity of the detection depends on the accuracy of the differential photometric measurements of binary components. Unresolved companions up to seven magnitudes fainter than the primary are detectable in the BVRI photometric system.

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