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Empirical bolometric correction coefficients for nearby main-sequence stars in the Gaia era

dc.contributor.authorKose, Y.
dc.contributor.authorBakış, Volkan
dc.contributor.authorAliçavuş, Fahri
dc.contributor.authorÖzer, Şule
dc.contributor.authorAlpsoy, M.
dc.contributor.authorAslan, Gülçin Ece
dc.contributor.authorEker, Zeki
dc.contributor.authorSoydugan, Faruk
dc.contributor.authorBilir, Selçuk
dc.date.accessioned2021-03-02T17:32:15Z
dc.date.available2021-03-02T17:32:15Z
dc.identifier.citationEker Z., Soydugan F., Bilir S., Bakış V., Aliçavuş F., Özer Ş., Aslan G. E. , Alpsoy M., Kose Y., "Empirical bolometric correction coefficients for nearby main-sequence stars in the Gaia era", MONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY, cilt.496, ss.3887-3905, 2020
dc.identifier.issn0035-8711
dc.identifier.othervv_1032021
dc.identifier.otherav_3af57415-7717-4ee3-8f56-0f573b5acdc6
dc.identifier.urihttp://hdl.handle.net/20.500.12627/3964
dc.identifier.urihttps://doi.org/10.1093/mnras/staa1659
dc.description.abstractNearby detached double-lined eclipsing binaries with most accurate data were studied and 290 systems were found with at least one main-sequence component having a metallicity of 0.008 10 000 K, while the quadratic relation is valid for T-eff < 10 000 K; that is, both are valid in the same temperature range in which the BC-Teff relation is valid. New BCs computed from Teff and other astrophysical parameters are tabulated, as well.
dc.language.isoeng
dc.subjectFizik
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.subjectUzay bilimi
dc.subjectTemel Bilimler (SCI)
dc.titleEmpirical bolometric correction coefficients for nearby main-sequence stars in the Gaia era
dc.typeMakale
dc.relation.journalMONTHLY NOTICES OF THE ROYAL ASTRONOMICAL SOCIETY
dc.contributor.departmentAkdeniz Üniversitesi , Fen Fakültesi , Uzay Bilimleri Ve Teknolojileri
dc.identifier.volume496
dc.identifier.startpage3887
dc.identifier.endpage3905
dc.contributor.firstauthorID2273725


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