KR Cygni: a near-contact eclipsing binary?

Details KR Cygni: a near-contact eclipsing binary? KR Cygni: a near-contact eclipsing binary?

Sep 2004

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2004ap%26ss.293..307s&link_type=abstract

Astrophysics and Space Science, v. 293, Issue 3, p. 307-321 (2004).

Astronomy and Astrophysics

Astrophysics

2

Eclipsing Binaries, Near-Contact Systems

Scientific paper

In this study we present photometric observations of the eclipsing binary KR Cyg made in 1999 and 2000. The observations of the eclipsing binary KR Cyg have been carried out in B, V and R colours at the Ege University Observatory. A new seasonal light curves are presented. New times of minima and ephemerides are given. Based on a statistical analysis of the times of minima obtained by photoelectric photometry, the orbital period of the system is found to be constant. The photometric mass ratio of the system is well determined. The corresponding light curves were analyzed by the Wilson-Devinney code.

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