Apsidal Motion of Two Eclipsing Binaries: V796 Cyg and V2783 Ori

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dc.contributor.authorBulut, A.
dc.contributor.authorBulut, I.
dc.contributor.authorCicek, C.
dc.contributor.authorErdem, A.
dc.date.accessioned2025-01-27T21:07:13Z
dc.date.available2025-01-27T21:07:13Z
dc.date.issued2017
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description32nd International Physics Congress of Turkish-Physical-Society (TPS) -- SEP 06-09, 2016 -- Bodrum, TURKEY
dc.description.abstractIn 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.
dc.description.sponsorshipTurkish Phys Soc
dc.identifier.doi10.1063/1.4976439
dc.identifier.isbn978-0-7354-1483-9
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85016039402
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.4976439
dc.identifier.urihttps://hdl.handle.net/20.500.12428/27930
dc.identifier.volume1815
dc.identifier.wosWOS:000435205100095
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofProceedings of The Turkish Physical Society 32nd International Physics Congress (Tps32)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectEclipsing binary stars
dc.subjectapsidal motion
dc.subjectindividual: V796 Cyg and V278.1 Ori
dc.titleApsidal Motion of Two Eclipsing Binaries: V796 Cyg and V2783 Ori
dc.typeConference Object

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