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dc.contributor.authorSaral, G.
dc.contributor.authorTerzioglu, Z.
dc.contributor.authorGokay, G.
dc.contributor.authorGursoytrak, S. H.
dc.contributor.authorCerit, S.
dc.contributor.authorGurol, B.
dc.date.accessioned2021-03-03T19:05:18Z
dc.date.available2021-03-03T19:05:18Z
dc.identifier.citationGurol B., Gokay G., Saral G., Gursoytrak S. H. , Cerit S., Terzioglu Z., "Absolute and geometric parameters of contact binary GW Cnc", NEW ASTRONOMY, cilt.46, ss.31-39, 2016
dc.identifier.issn1384-1076
dc.identifier.othervv_1032021
dc.identifier.otherav_52aabeb9-b853-477f-ac32-56375d83d062
dc.identifier.urihttp://hdl.handle.net/20.500.12627/58673
dc.identifier.urihttps://doi.org/10.1016/j.newast.2015.12.002
dc.description.abstractWe present the results of our investigation on the geometrical and physical parameters of the W UMa type binary system GW Cnc. We analyzed the photometric data obtained in 2010 and 2011 at Ankara University Observatory (AUO) and the spectroscopic data obtained in 2010 at TUBITAK National Observatory (TUG) by using the Wilson-Devinney (2013 revision) code to obtain the absolute and geometrical parameters. We derived masses and radii of the eclipsing system to be M-1 = 0.257 M-circle dot, M-2 = 0.971 M-circle dot, R-1 = 0.526 R-circle dot and R-2 = 0.961 R-circle dot with an orbital inclination i(degrees) = 83.38 +/- 0.25 and we determined the GW Cnc system to be a W-type W UMa over-contact binary with a mass ratio of q = 3.773 +/- 0.007. (C) 2015 Elsevier B.V. All rights reserved.
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleAbsolute and geometric parameters of contact binary GW Cnc
dc.typeMakale
dc.relation.journalNEW ASTRONOMY
dc.contributor.departmentAnkara Üniversitesi , ,
dc.identifier.volume46
dc.identifier.startpage31
dc.identifier.endpage39
dc.contributor.firstauthorID233797


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