A photometric study of the recently discovered eclipsing binary V776 Cassiopeiae

Details A photometric study of the recently discovered eclipsing binary V776 Cassiopeiae A photometric study of the recently discovered eclipsing binary V776 Cassiopeiae

Dec 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004aspc..318..192e&link_type=abstract

In Spectroscopically and Spatially Resolving the Components of the Close Binary Stars, Proceedings of the Workshop held 20-24 Oc

Astronomy and Astrophysics

Astronomy

Scientific paper

Photoelectric U, B, and V light curves of the recently discovered eclipsing binary V776 Cas were analyzed to determine the preliminary physical parameters of the system by using the Djurašević's (1992a) inverse-problem method. The light curves which have an amplitude of about 0.15 arcmin were obtained at the TÜBITAK National Observatory (TUG) between 8 and 9 October 2002. The analysis yields an A-type contact binary as a high overcontact configuration. Due to the proximity of its visual companion the light curves were contaminated by the third-light effect which has a relatively small influence on the estimation of the system parameters.

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