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AM Leo'nun Fotometrik Analizi

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dc.contributor.authorEminoğlu, Fatma Başak
dc.contributor.authorKabadayı, Özge
dc.contributor.authorYelkenci, Fuat Korhan
dc.date.accessioned2014-08-11T14:29:10Z
dc.date.available2014-08-11T14:29:10Z
dc.date.issued2005-11
dc.description.abstractUBV light curves of AM Leo which is a short period W UMa type contact binary were obtained at Ankara University Observatory in 2005 and analyzed. Preliminary solutions of physical parameters of the system were carried out by using Binary Maker and Nightfall lightcurve analysis programs. Two different solutions were determined by adjusting and by fixing the mass ratio (q = 2.51). The solutions describe that AM Leo system has a W sub-type overcontact configuration with an inclination of - 82° and a very small temperature differences of the components.en
dc.identifier.issn1303-2739
dc.identifier.urihttp://hdl.handle.net/11413/332
dc.language.isotrtr_TR
dc.publisherİstanbul Kültür Üniversitesi Yayınlarıtr_TR
dc.subjectÖrten Çift Yıldızlartr_TR
dc.subjectIşık Eğrisi Analiztr_TR
dc.subjectAM Leotr_TR
dc.subjectEclipsing Binary Starstr_TR
dc.subjectLight Curve Analysistr_TR
dc.titleAM Leo'nun Fotometrik Analizitr_TR
dc.typeArticle
dspace.entity.typePublication

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Cilt 3, Sayı 3, Kasım 2005