BVR Photometric Analysis of GSC 4277-0586 and GSC 3152-1202

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dc.contributor.authorBulut, I.
dc.contributor.authorBulut, A.
dc.date.accessioned2025-01-27T20:27:03Z
dc.date.available2025-01-27T20:27:03Z
dc.date.issued2015
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractA detailed light curve analysis of the newly discovered eccentric orbit eclipsing binaries GSC 4277-0586 and GSC 3152-1202 are presented for the fist time. For both systems, the B, V and R light curves were secured and also new minima times have been derived. The analysis was made using the Wilson-Devinney program. The absolute dimensions were calculated using mass-luminosity relation for main sequence stars. The O - C diagram of GSC 3152-1202 was also analyzed using all reliable times of minima and the elements of apsidal motion were computed. The apsidal motion period has been found to be 36.6 perpendicular to 9.8 years.
dc.identifier.endpage138
dc.identifier.issn0001-5237
dc.identifier.issue1
dc.identifier.scopus2-s2.0-84927712941
dc.identifier.scopusqualityQ2
dc.identifier.startpage127
dc.identifier.urihttps://hdl.handle.net/20.500.12428/22564
dc.identifier.volume65
dc.identifier.wosWOS:000353551700007
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherCopernicus Foundation Polish Astronomy
dc.relation.ispartofActa Astronomica
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectbinaries: eclipsing
dc.subjectStars: fundamental parameters
dc.subjectStars: individual: GSC 4277-0586, GSC 3152-1202
dc.titleBVR Photometric Analysis of GSC 4277-0586 and GSC 3152-1202
dc.typeArticle

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