Apsidal Motion of Two Eclipsing Binaries: V796 Cyg and V2783 Ori
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Tarih
2017
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Amer Inst Physics
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
In this study, the orbital period variations of two eclipsing binary systems showing apsidal motion were studied. Their O - C diagrams were analysed using all reliable eclipse timings and the elements of apsidal motion of two systems were improved. We found periods of apsidal motion of V796 Cyg and V2783 Ori to be 32.7 +/- 0.2 years and 415 +/- 50 years, respectively.
Açıklama
32nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEY
Anahtar Kelimeler
Eclipsing binary stars, apsidal motion, individual: V796 Cyg and V278.1 Ori
Kaynak
Proceedings of The Turkish Physical Society 32nd International Physics Congress (Tps32)
WoS Q Değeri
N/A
Scopus Q Değeri
Q4
Cilt
1815
