KR Cygni: A near-contact eclipsing binary?
Articles > Article · 2004
Authors: Esin SİPAHİ KILIÇ, O GULMEN
ASTROPHYSICS AND SPACE SCIENCE, Journal Indexed in SCI Expanded, International, 2004, vol 293, pp 307-321
DOI: 10.1023/b:astr.0000044305.71006.1b
Summary
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.