The Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way

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dc.authoridYaz Gokce, Esma/0000-0003-0958-2935
dc.authoridSoydugan, Faruk/0000-0002-5141-7645
dc.authoridBilir, Selcuk/0000-0003-3510-1509
dc.contributor.authorEker, Z.
dc.contributor.authorBilir, S.
dc.contributor.authorSoydugan, Faruk
dc.contributor.authorGokce, E. Yaz
dc.contributor.authorSoydugan, Esin
dc.contributor.authorTuysuz, M.
dc.contributor.authorSenyuz, T.
dc.date.accessioned2025-01-27T20:44:00Z
dc.date.available2025-01-27T20:44:00Z
dc.date.issued2014
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
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.description.sponsorshipScientific and Technological Research Council of Turkey (TUBITAK) [106T688, 111T224]
dc.description.sponsorshipThis work has been supported in part by the Scientific and Technological Research Council of Turkey (TUBITAK) grant numbers 106T688 and 111T224. Authors would like to thank anonymous referee who provided valuable comments for improving the manuscript and Mr. Muzaffer Karasulu for proof reading. This research has made use of the SIMBAD database, operated at CDS, Strasbourg, France and NASA's Astrophysics Data System. We would like to thank Dr. Nilda Oklay for helping online material.
dc.identifier.doi10.1017/pasa.2014.17
dc.identifier.issn1323-3580
dc.identifier.issn1448-6083
dc.identifier.scopus2-s2.0-84901493200
dc.identifier.scopusqualityQ1
dc.identifier.urihttps://doi.org/10.1017/pasa.2014.17
dc.identifier.urihttps://hdl.handle.net/20.500.12428/24449
dc.identifier.volume31
dc.identifier.wosWOS:000339714300003
dc.identifier.wosqualityQ2
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherCambridge Univ Press
dc.relation.ispartofPublications of The Astronomical Society of Australia
dc.relation.publicationcategoryinfo:eu-repo/semantics/openAccess
dc.rightsinfo:eu-repo/semantics/openAccess
dc.snmzKA_WoS_20250125
dc.subjectastronomical data based: catalogues
dc.subjectstars: binaries: eclipsing
dc.subjectstars: fundamental parameters
dc.subjectstars: binaries: spectroscopic
dc.titleThe Catalogue of Stellar Parameters from the Detached Double-Lined Eclipsing Binaries in the Milky Way
dc.typeArticle

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