Apsidal Motion in Eclipsing Binary GG Orionis

Basit Öğe Kaydı
dc.contributor.authorYilan, E.
dc.contributor.authorBulut, I.
dc.date.accessioned2025-01-27T20:49:35Z
dc.date.available2025-01-27T20:49:35Z
dc.date.issued2016
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description9th International Physics Conference of the Balkan-Physical-Union (BPU) -- AUG 24-27, 2015 -- Istanbul Univ, Beyazit Campus, Istanbul, TURKEY
dc.description.abstractThe 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.
dc.description.sponsorshipBalkan Phys Union,Turkish Phys Soc
dc.identifier.doi10.1063/1.4944141
dc.identifier.isbn978-0-7354-1369-6
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-84984541351
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4944141
dc.identifier.urihttps://hdl.handle.net/20.500.12428/25230
dc.identifier.volume1722
dc.identifier.wosWOS:000375923300022
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartof9th International Physics Conference of The Balkan Physical Union (Bpu-9)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectOri
dc.subjectSystems
dc.titleApsidal Motion in Eclipsing Binary GG Orionis
dc.typeConference Object

Dosyalar

Koleksiyon

WoS İndeksli Yayınlar Koleksiyonu
Scopus İndeksli Yayınlar Koleksiyonu