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Monitoring secular orbital period variations of some eclipsing binaries at the Ankara University Observatory

dc.contributor.authorAk, Tansel
dc.contributor.authorSELAM, S. O.
dc.contributor.authorYUCE, K.
dc.contributor.authorAlbayrak, Büşra
dc.date.accessioned2021-03-03T14:17:09Z
dc.date.available2021-03-03T14:17:09Z
dc.identifier.citationYUCE K., SELAM S. O. , Albayrak B., Ak T., "Monitoring secular orbital period variations of some eclipsing binaries at the Ankara University Observatory", ASTROPHYSICS AND SPACE SCIENCE, cilt.304, ss.67-69, 2006
dc.identifier.issn0004-640X
dc.identifier.othervv_1032021
dc.identifier.otherav_38c2851d-9565-4646-8d71-5437d3845804
dc.identifier.urihttp://hdl.handle.net/20.500.12627/42231
dc.identifier.urihttps://doi.org/10.1007/s10509-006-9076-1
dc.description.abstractThis study concerns the long-term monitoring of the secular variation character in the orbital period of some short-period eclipsing binaries observed at the Ankara University Observatory. Among the systems of our observing list are CK Boo, V502 Oph and V836 Cyg that show long-term secular variations in their orbital periods. We use classical O-C diagram analysis technique as a tool to reveal the character of the period variations of these binary systems.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleMonitoring secular orbital period variations of some eclipsing binaries at the Ankara University Observatory
dc.typeMakale
dc.relation.journalASTROPHYSICS AND SPACE SCIENCE
dc.contributor.departmentAnkara Üniversitesi , ,
dc.identifier.volume304
dc.identifier.startpage67
dc.identifier.endpage69
dc.contributor.firstauthorID53894


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