Photometric analysis of the eclipsing binary V1425 Cygni

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

ASTROPHYSICS AND SPACE SCIENCE, vol.241, no.2, pp.327-332, 1996 (SCI-Expanded) identifier identifier

  • Publication Type: Article / Article
  • Volume: 241 Issue: 2
  • Publication Date: 1996
  • Doi Number: 10.1007/bf00645233
  • Journal Name: ASTROPHYSICS AND SPACE SCIENCE
  • Journal Indexes: Science Citation Index Expanded (SCI-EXPANDED), Scopus
  • Page Numbers: pp.327-332
  • Çanakkale Onsekiz Mart University Affiliated: No

Abstract

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.