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New period study of the eclipsing binary V865 Cygni
Authors:Petr Molík  Marek Wolf  Miloslav Zejda
Institution:(1) 392 01 Soběslav, Okružní 103, Czech Republic;(2) Astronomical Institute, Charles University Prague, V Holešovičkách 2, 180 00 Prague, Czech Republic;(3) Institute of Theoretical Physics and Astrophysics, Masaryk University, 611 37 Brno, Czech Republic
Abstract:Several new precise times of minima, based on CCD observations, have been secured for the relatively seldom studied eclipsing binary V865 Cyg (P=0d.365 days). Its OC diagram was analysed and new light elements are given. We showed that there is probably no parabolic period increase in V865 Cyg. Instead, a single abrupt period increase can be distinguished in the OC diagram.
Keywords:Star: eclipsing binary  Star: individual: V865 Cyg
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