New period study of the eclipsing binary V865 Cygni

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Authors	MOLÍK Petr WOLF Marek ZEJDA Miloslav
Year of publication	2007
Type	Article in Periodical
Magazine / Source	Astrophysics and Space Science
MU Faculty or unit	Faculty of Science
Citation
web	http://adsabs.harvard.edu/abs/2007Ap%26SS.310..149M
Field	Astronomy and astrophysics
Keywords	eclipsing binary; period;O-C;
Description	Several new precise times of minima, based on CCD observations, have been secured for the relatively seldom studied eclipsing binary V865 Cyg (P=0.365 days). Its O-C 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 O-C diagram.
Related projects:	New approaches to variable stars data processing and interpretation Fotometrický výzkum zákrytových dvojhvězd