Properties of the Main-Sequence Eclipsing Binary Uz Draconis

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dc.contributor.authorLacy, Ch
dc.contributor.authorGulmen, O
dc.contributor.authorGudur, N
dc.contributor.authorSezer, C
dc.date.accessioned2019-10-27T11:37:03Z
dc.date.available2019-10-27T11:37:03Z
dc.date.issued1989
dc.departmentEge Üniversitesien_US
dc.identifier.doi10.1086/115028
dc.identifier.endpage835en_US
dc.identifier.issn0004-6256
dc.identifier.issn0004-6256en_US
dc.identifier.issue3en_US
dc.identifier.startpage822en_US
dc.identifier.urihttps://doi.org/10.1086/115028
dc.identifier.urihttps://hdl.handle.net/11454/34058
dc.identifier.volume97en_US
dc.identifier.wosWOS:A1989T407400020en_US
dc.identifier.wosqualityN/Aen_US
dc.indekslendigikaynakWeb of Scienceen_US
dc.language.isoenen_US
dc.publisherAmer Inst Physicsen_US
dc.relation.ispartofAstronomical Journalen_US
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanıen_US
dc.rightsinfo:eu-repo/semantics/openAccessen_US
dc.titleProperties of the Main-Sequence Eclipsing Binary Uz Draconisen_US
dc.typeArticleen_US

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