Photometric-Study of the Eclipsing Binary V-1073 Cygni

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dc.contributor.authorSezer, C
dc.date.accessioned2019-10-27T11:35:50Z
dc.date.available2019-10-27T11:35:50Z
dc.date.issued1993
dc.departmentEge Üniversitesien_US
dc.description.abstractPhotoelectric observations of the eclipsing binary V 1073 Cyg have been carried out in B and V colours at the Ege University Observatory. The light curves were analyzed with the Wilson-Devinney approach. A period study reveals that the orbital period of the system is decreasing at the rate of (3.21 +/- 0.17) second per century.en_US
dc.identifier.doi10.1007/BF00658129
dc.identifier.endpage31en_US
dc.identifier.issn0004-640X
dc.identifier.issn0004-640Xen_US
dc.identifier.issue1en_US
dc.identifier.startpage15en_US
dc.identifier.urihttps://doi.org/10.1007/BF00658129
dc.identifier.urihttps://hdl.handle.net/11454/33793
dc.identifier.volume208en_US
dc.identifier.wosWOS:A1993MR94800003en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.language.isoenen_US
dc.publisherKluwer Academic Publen_US
dc.relation.ispartofAstrophysics and Space Scienceen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/closedAccessen_US
dc.titlePhotometric-Study of the Eclipsing Binary V-1073 Cygnien_US
dc.typeArticleen_US

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