Photometric study of close binary stars in the M35, M67, and M71 Galactic clusters

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dc.contributor.authorKocak, D.
dc.contributor.authorIcli, T.
dc.contributor.authorYakut, K.
dc.date.accessioned2020-12-01T12:05:27Z
dc.date.available2020-12-01T12:05:27Z
dc.date.issued2020
dc.departmentEge Üniversitesien_US
dc.description.abstractWe obtained new multicolour photometry of close binary stars in the young open cluster M35, the solar-age open cluster M67, and the globular cluster M71. New observations have been carried out at the TUBITAK National Observatory (TUG) by using the 100 cm (T100) telescope. We present observational results for eclipsing binary systems in the selected Galactic clusters. New accurate light curves for 2MASS J19532554 + 1851175, 2MASS J19533427 + 1844047, 2MASS J06092044 + 2415155, and AH Cnc were obtained. We analysed the light curves and derived some of the orbital parameters of the systems.en_US
dc.description.sponsorshipTurkish Scientific and Research Council (TUBITAK)Turkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK) [117F188]; TUBITAK National ObservatoryTurkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK) [18CT1001422]; TUBITAKTurkiye Bilimsel ve Teknolojik Arastirma Kurumu (TUBITAK) [2211-C, 2214]; COST (European Cooperation in Science and Technology) ActionEuropean Cooperation in Science and Technology (COST) [CA15117, CA16104]en_US
dc.description.sponsorshipWe are grateful to the anonymous reviewers for their comments and suggestions. This study was supported by Turkish Scientific and Research Council (TUBITAK 117F188) and the TUBITAK National Observatory (18CT1001422). DK thanks TUBITAK for his Fellowship (2211-C and 2214). KY would like to acknowledge the contribution of COST (European Cooperation in Science and Technology) Action CA15117 and CA16104.en_US
dc.identifier.doi10.31577/caosp.2020.50.2.508
dc.identifier.endpage512en_US
dc.identifier.issn1335-1842
dc.identifier.issn1336-0337
dc.identifier.issn1335-1842en_US
dc.identifier.issn1336-0337en_US
dc.identifier.issue2en_US
dc.identifier.scopus2-s2.0-85087083088en_US
dc.identifier.scopusqualityQ3en_US
dc.identifier.startpage508en_US
dc.identifier.urihttps://doi.org/10.31577/caosp.2020.50.2.508
dc.identifier.urihttps://hdl.handle.net/11454/62999
dc.identifier.volume50en_US
dc.identifier.wosWOS:000523574300027en_US
dc.identifier.wosqualityQ4en_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.indekslendigikaynakScopusen_US
dc.language.isoenen_US
dc.publisherSlovak Academy Sciences Astronomical Insten_US
dc.relation.ispartofContributions of the Astronomical Observatory Skalnate Plesoen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.subjectstars: binaries: closeen_US
dc.subjectclusters: openen_US
dc.subjectclusters: globularen_US
dc.titlePhotometric study of close binary stars in the M35, M67, and M71 Galactic clustersen_US
dc.typeArticleen_US

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