Isochronal Ages of Some Eclipsing Binary Stars with Eccentric Orbits

dc.contributor.authorBulut, İbrahim
dc.contributor.authorGüneş, Mümin
dc.date.accessioned2025-01-27T19:04:28Z
dc.date.available2025-01-27T19:04:28Z
dc.date.issued2022
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description.abstractIsochronal ages of the 32 eclipsing binary stars with eccentric orbits from the catalog of Bulut and Demircan (2007) were computed using the Y2 stellar evolution models. First, we derived the metallicity Z-values from evolutionary sequences. Then, using these metallicity in the Y2 models, a set of isochrones were computed. Lastly, the ages were found from the isochrone that was best-fitting the locations of both components. 19 of the 32 ages were calculated with a 20% accuracy. These were compared with the circularization times-scales. © 2022, Institute of Astronomy and Rozhen NAO. All rights reserved.
dc.identifier.issn1313-2709
dc.identifier.scopus2-s2.0-85122153088
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://hdl.handle.net/20.500.12428/13964
dc.identifier.volume36
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherInstitute of Astronomy and Rozhen NAO
dc.relation.ispartofBulgarian Astronomical Journal
dc.relation.publicationcategoryMakale - Uluslararası Hakemli Dergi - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_Scopus_20250125
dc.subjectStars: binaries; Stars: binaries: eclipsing; Stars: evolution
dc.titleIsochronal Ages of Some Eclipsing Binary Stars with Eccentric Orbits
dc.typeArticle

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