The early type contact binary system V 382 Cygni

Degirmenci O., Sezer C., Demircan O., Erdem A., Ozdemir S., AK H., ...Daha Fazla

ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES, cilt.134, sa.2, ss.327-331, 1999 (SCI-Expanded) identifier identifier

  • Yayın Türü: Makale / Tam Makale
  • Cilt numarası: 134 Sayı: 2
  • Basım Tarihi: 1999
  • Doi Numarası: 10.1051/aas:1999143
  • Dergi Adı: ASTRONOMY & ASTROPHYSICS SUPPLEMENT SERIES
  • Derginin Tarandığı İndeksler: Science Citation Index Expanded (SCI-EXPANDED)
  • Sayfa Sayıları: ss.327-331
  • Anahtar Kelimeler: stars : binaries : eclipsing, stars : individual : V 382 Cyg, ECLIPSING BINARIES, O-STARS, MASSES, CEP
  • Ankara Üniversitesi Adresli: Evet

Özet

New photometric data set of the early type contact binary V382 Cyg have been analyzed with emphasis on determining the photometric mass ratio of the system. The result (q = 0.68) supports the value given by Popper & Hill (1991). A study of the system using new data shows a period increase of about 3.28 s per century, which corresponds to a very large rate similar to 5.0 10(-6) M./yr of mass transfer from the less massive to the more massive component under the conservative mass transfer hypothesis.