Differential UBV photometry of the eclipsing binary SVS 2086

Details Differential UBV photometry of the eclipsing binary SVS 2086 Differential UBV photometry of the eclipsing binary SVS 2086

Apr 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985ap%26ss.111..123c&link_type=abstract

Astrophysics and Space Science (ISSN 0004-640X), vol. 111, no. 1, April 1985, p. 123-129.

Astronomy and Astrophysics

Astrophysics

4

Eclipsing Binary Stars, Stellar Spectrophotometry, Ubv Spectra, Astronomical Coordinates, Light Curve, Stellar Evolution

Scientific paper

Photoelectric UBV differential observations of the eclipsing binary SVS
2086 are presented. The system shows a W UMa-type light curve, with an
amplitude of 0.5 in V light; the period seems to be longer than
previously believed.

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