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dc.contributor.authorErdem, Ahmet
dc.contributor.authorDeğirmenci, Ömer Lütfi
dc.contributor.authorBozkurt, Zeynep
dc.contributor.authorYakut, Kadri
dc.contributor.authorEsenoglu, Hasan Hüseyin
dc.contributor.authorBulut, İbrahim
dc.contributor.authorDemircan, Osman
dc.contributor.authorBudding, Edwin
dc.contributor.authorÇiçek, Caner
dc.contributor.authorSoydugan, F
dc.contributor.authorSoydugan, E
dc.date.accessioned2021-03-03T19:34:56Z
dc.date.available2021-03-03T19:34:56Z
dc.date.issued2005
dc.identifier.citationBulut İ., Demircan O., Budding E., Erdem A., Çiçek C., Esenoglu H. H. , Soydugan F., Soydugan E., Değirmenci Ö. L. , Bozkurt Z., et al., "Photometric study of the binary system V397 cephei", PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN, cilt.57, sa.2, ss.335-339, 2005
dc.identifier.issn0004-6264
dc.identifier.othervv_1032021
dc.identifier.otherav_5558b275-7faa-483b-aec9-170750643864
dc.identifier.urihttp://hdl.handle.net/20.500.12627/60338
dc.identifier.urihttps://doi.org/10.1093/pasj/57.2.335
dc.description.abstractThe first ground-based UBV observations (2001, Inf. Bull. Variable Stars, 5129) of V397 Cep were analyzed by using the Wilson-Devinney method, and the results were compared with others in the literature. A consistent geometry with a photometric mass-ratio close to unity and an eccentric orbit of e similar or equal to 0.13 was found. The longitude of the periastron (omega) was found significantly different for two different light curves, which is strongly suggestive of an apsidal motion with a period of about 300 yr. This makes V397 Cep an important candidate for studies of apsidal motion.
dc.language.isoeng
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titlePhotometric study of the binary system V397 cephei
dc.typeMakale
dc.relation.journalPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF JAPAN
dc.contributor.departmentÇanakkale Onsekiz Mart Üniversitesi , ,
dc.identifier.volume57
dc.identifier.issue2
dc.identifier.startpage335
dc.identifier.endpage339
dc.contributor.firstauthorID40504


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