Apsidal Motion in Eclipsing Binary GG Orionis
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Tarih
2016
Dergi Başlığı
Dergi ISSN
Cilt Başlığı
Yayıncı
Amer Inst Physics
Erişim Hakkı
info:eu-repo/semantics/closedAccess
Özet
The study of apsidal motion in binary stars with eccentric orbit is well known as an important source of information for the stellar internal structure as well as the possibility of verification of general relativity. In this study, the apsidal motion of the eccentric eclipsing binary GG Ori (P = 6.631 days, e = 0.22) has been analyzed using the times of minimum light taken from the literature and databases and the elements of apsidal motion have been computed. The method described by Gimenez and Garcia-Pelayo (1983) has been used for the apsidal motion analysis.
Açıklama
9th International Physics Conference of the Balkan-Physical-Union (BPU) -- AUG 24-27, 2015 -- Istanbul Univ, Beyazit Campus, Istanbul, TURKEY
Anahtar Kelimeler
Ori, Systems
Kaynak
9th International Physics Conference of The Balkan Physical Union (Bpu-9)
WoS Q Değeri
N/A
Scopus Q Değeri
Q4
Cilt
1722
