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Paper: A Photometric Study of the Recently Discovered Eclipsing Binary V776 Cassiopeiae
Volume: 318, Spectroscopically and Spatially Resolving the Components of Close Binary Stars
Page: 192
Authors: Elmasli, A.; Tanriverdi, T.; Albayrak, B.; Selam, S.O.; Djurasevic, G.
Abstract: 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 0.15m were obtained at the TÜBİTAK 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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