Physical parameters of some close binaries: ET Boo, V1123 Tau, V1191 Cyg, V1073 Cyg and V357 Peg

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dc.authorid0000-0001-6947-822X
dc.contributor.authorEkmekci, F.
dc.contributor.authorElmasli, A.
dc.contributor.authorYilmaz, M.
dc.contributor.authorKilicoglu, T.
dc.contributor.authorTanriverdi, T.
dc.contributor.authorBasturk, O.
dc.contributor.authorSelam, S. O.
dc.date.accessioned2019-08-01T13:38:39Z
dc.date.available2019-08-01T13:38:39Z
dc.date.issued2012
dc.departmentNiğde ÖHÜ
dc.description.abstractWith the aim of providing new and up-to-date absolute parameters of some close binary systems, new BVR CCD photometry was carried out at the Ankara University Observatory (AUG) for five eclipsing binaries, ET Boo, V1123 Tau, V1191 Cyg, V1073 Cyg and V357 Peg between April, 2007 and October, 2008. In this paper, we present the orbital solutions for these systems obtained by simultaneous light and radial velocity curve analyses. Extensive orbital solution and absolute parameters for ET Boo system were given for the first time through this study. According to the analyses, ET Boo is a detached binary while the parameters of four remaining systems are consistent with the nature of contact binaries. The evolutionary status of the components of these systems are also discussed by referring to their absolute parameters found in this study. (C) 2012 Elsevier B.V. All rights reserved.
dc.description.sponsorshipScientific and Technological Research Council of Turkey (TUBITAK) [BIDEB-2211]
dc.description.sponsorshipThis research has made use of the Simbad database, operated at CDS, Strasbourg, France, and of NASA's Astrophysics Data System Bibliographic Services. OB would like to thank The Scientific and Technological Research Council of Turkey (TUBITAK) for their support through BIDEB-2211 scholarship.
dc.identifier.doi10.1016/j.newast.2012.03.001
dc.identifier.endpage609
dc.identifier.issn1384-1076
dc.identifier.issue7
dc.identifier.scopus2-s2.0-84861564669
dc.identifier.scopusqualityQ3
dc.identifier.startpage603
dc.identifier.urihttps://dx.doi.org/10.1016/j.newast.2012.03.001
dc.identifier.urihttps://hdl.handle.net/11480/4539
dc.identifier.volume17
dc.identifier.wosWOS:000305375200001
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.institutionauthor[0-Belirlenecek]
dc.language.isoen
dc.publisherELSEVIER SCIENCE BV
dc.relation.ispartofNEW ASTRONOMY
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.subjectBinaries: eclipsing
dc.subjectStars: fundamental parameters
dc.subjectStars: individual (ET Boo, V1123 Tau, V1191 Cyg, V1073 Cyg, V357 Peg)
dc.titlePhysical parameters of some close binaries: ET Boo, V1123 Tau, V1191 Cyg, V1073 Cyg and V357 Peg
dc.typeArticle

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