New period study of the eclipsing binary V865 Cygni

Details New period study of the eclipsing binary V865 Cygni New period study of the eclipsing binary V865 Cygni

Jul 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007ap%26ss.310..149m&link_type=abstract

Astrophysics and Space Science, Volume 310, Issue 1-2, pp. 149-152

Astronomy and Astrophysics

Astrophysics

Star: Eclipsing Binary, Star: Individual: V865&Nbsp, Cyg

Scientific paper

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 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.

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