Photometric analysis of the eclipsing binary V1425 Cygni

DEGIRMENCI O., GULMEN O., SEZER C., GUDUR N., Erdem A.

ASTROPHYSICS AND SPACE SCIENCE, cilt.241, sa.2, ss.327-332, 1996 (SCI-Expanded) identifier identifier

  • 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.