Apsidal Motion in Eclipsing Binaries: FT Ori and MZ Lac
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Tarih
2016
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Amer Inst Physics
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
In this study, the apsidal motion analysis of two eccentric eclipsing binaries, FT Ori (P = 3.150 days, e = 0.397) and MZ Lac (P = 3.158 days, e = 0.399), have been presented. Their O - C diagrams were studied using all reliable times of minima found in the literature and new values for the elements of the apsidal motion for two systems have been computed. We found long periods of apsidal motion of 538 +/- 12 years and 424 +/- 6 years for FT Ori and MZ Lac, respectively.
Açıklama
9th International Physics Conference of the Balkan-Physical-Union (BPU) -- AUG 24-27, 2015 -- Istanbul Univ, Beyazit Campus, Istanbul, TURKEY
Anahtar Kelimeler
Eclipsing binary stars, apsidal motion, individual: FT Ori and MZ Lac
Kaynak
9th International Physics Conference of The Balkan Physical Union (Bpu-9)
WoS Q Değeri
N/A
Scopus Q Değeri
Q4
Cilt
1722
