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dc.contributor.authorTüysüz, Mehmet
dc.contributor.authorGokce, E. Yaz
dc.contributor.authorSoydugan, Esin
dc.contributor.authorSenyuz, T.
dc.contributor.authorDemircan, Oya
dc.contributor.authorEker, Zeki
dc.contributor.authorBilir, Selçuk
dc.contributor.authorSoydugan, Faruk
dc.date.accessioned2021-03-03T08:56:52Z
dc.date.available2021-03-03T08:56:52Z
dc.identifier.citationEker Z., Bilir S., Soydugan F., Gokce E. Y. , Soydugan E., Tüysüz M., Senyuz T., Demircan O., "The Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way", PUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA, cilt.31, 2014
dc.identifier.issn1323-3580
dc.identifier.othervv_1032021
dc.identifier.otherav_1a5f9edb-e55b-4062-9e70-4a7d176d703a
dc.identifier.urihttp://hdl.handle.net/20.500.12627/23013
dc.identifier.urihttps://doi.org/10.1017/pasa.2014.17
dc.description.abstractThe most accurate stellar astrophysical parameters were collected from the solutions of the light and the radial velocity curves of 257 detached double-lined eclipsing binaries in the Milky Way. The catalogue contains masses, radii, surface gravities, effective temperatures, luminosities, projected rotational velocities of the component stars, and the orbital parameters. The number of stars with accurate parameters increased 67% in comparison to the most recent similar collection by Torres, Andersen, & Gimenez (2010). Distributions of some basic parameters were investigated. The ranges of effective temperatures, masses, and radii are 2 750 < T-eff (K)< 43 000, 0.18 < M/M-circle dot < 33, and 0.2 < R/R-circle dot < 21.2, respectively. Being mostly located in one kpc in the Solar neighborhood, the present sample covers distances up to 4.6 kpc within the two local Galactic arms, Carina-Sagittarius and Orion Spur. The number of stars with both mass and radius measurements better than 1% uncertainty is 93, better than 3% uncertainty is 311, and better than 5% uncertainty is 388. It is estimated from the Roche lobe filling factors that 455 stars (88.5% of the sample) are spherical within 1% of uncertainty.
dc.language.isoeng
dc.subjectAstronomi ve Astrofizik
dc.subjectTemel Bilimler
dc.subjectFizik
dc.subjectTemel Bilimler (SCI)
dc.subjectUzay bilimi
dc.subjectASTRONOMİ VE ASTROFİZİK
dc.titleThe Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way
dc.typeMakale
dc.relation.journalPUBLICATIONS OF THE ASTRONOMICAL SOCIETY OF AUSTRALIA
dc.contributor.departmentAkdeniz Üniversitesi , Fen Fakültesi , Uzay Bilimleri Ve Teknolojileri
dc.identifier.volume31
dc.contributor.firstauthorID2219313


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