Photometric analysis of the eclipsing binary V1425 Cygni
Articles > Article · 1996
Authors: Ömer Lütfi DEĞİRMENCİ, O Gulmen, C Sezer, N Gudur, A Erdem
Astrophysics and Space Science, Journal Indexed in SCI Expanded, International, 1996, vol 241, pp 327-332
DOI: 10.1007/bf00645233
Summary
Photoelectric B and V light curves of the eclipsing binary V1425 Cygni were analyzed by the method of Wilson-Devinney. The system was found to be a semi-detached binary where the secondary component (less massive and cooler) fills its Roche lobe.