Photometric analysis of the eclipsing binary V1425 Cygni
ASTROPHYSICS AND SPACE SCIENCE, cilt.241, sa.2, ss.327-332, 1996 (SCI-Expanded)
- Yayın Türü: Makale / Tam Makale
- Cilt numarası: 241 Sayı: 2
- Basım Tarihi: 1996
- Doi Numarası: 10.1007/bf00645233
- Dergi Adı: ASTROPHYSICS AND SPACE SCIENCE
- Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED), Scopus
- Sayfa Sayıları: ss.327-332
- Çanakkale Onsekiz Mart Üniversitesi Adresli: Hayır
Özet
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.