Updated MS Luminosity-Radius-Temperature-Mass Relations for Solar Neighborhood Galactic Disk Stars

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dc.authoridSoydugan, Faruk/0000-0002-5141-7645
dc.authoridBAKIS, VOLKAN/0000-0002-3125-9010
dc.contributor.authorEker, Zeki
dc.contributor.authorBakis, Volkan
dc.contributor.authorBilir, Selcuk
dc.contributor.authorSoydugan, Faruk
dc.contributor.authorSteer, Ian
dc.contributor.authorSoydugan, Esin
dc.contributor.authorBakis, Hicran
dc.date.accessioned2025-01-27T20:11:45Z
dc.date.available2025-01-27T20:11:45Z
dc.date.issued2018
dc.departmentÇanakkale Onsekiz Mart Üniversitesi
dc.description34th International Physics Congress (IPS) of the Turkish-Physical-Society (TPS) -- SEP 05-09, 2018 -- Konacik, TURKEY
dc.description.abstractConventional mass- luminosity (M- L) relations are defined using 509 nearby main- sequence (MS) stars within the Solar neighborhood. A smooth mass- radius (M- R) relation was fixed from radii of MS stars appeared in literature having masses within the limits 0.179- 1.5 M. Similarly, a smooth mass- effective temperature (M- Teff) relation was derived for the main- sequence stars having masses within the limits 1.5- 31 M using their effective temperatures available. The omitted parts of M- R and M- Teff relations in the range from 0.179 to 31 M were computed according to Stephan- Boltzmann law, so inter- related M- L, M- R and M- Teff were achieved.
dc.description.sponsorshipTurkish Phys Soc
dc.description.sponsorshipScientific and Technological Research Council (TUBITAK) [114R072]; Akdeniz University BAP office
dc.description.sponsorshipThis study supported by the Scientific and Technological Research Council (TUBITAK) by the grant number 114R072. Thanks to Akdeniz University BAP office for providing partial support for this study.
dc.identifier.doi10.1063/1.5078888
dc.identifier.isbn978-0-7354-1768-7
dc.identifier.issn0094-243X
dc.identifier.scopus2-s2.0-85057161853
dc.identifier.scopusqualityQ4
dc.identifier.urihttps://doi.org/10.1063/1.5078888
dc.identifier.urihttps://hdl.handle.net/20.500.12428/20707
dc.identifier.volume2042
dc.identifier.wosWOS:000468358900016
dc.identifier.wosqualityN/A
dc.indekslendigikaynakWeb of Science
dc.indekslendigikaynakScopus
dc.language.isoen
dc.publisherAmer Inst Physics
dc.relation.ispartofTurkish Physical Society 34th International Physics Congress (Tps34)
dc.relation.publicationcategoryKonferans Öğesi - Uluslararası - Kurum Öğretim Elemanı
dc.rightsinfo:eu-repo/semantics/closedAccess
dc.snmzKA_WoS_20250125
dc.subjectcatalogues
dc.subjectbinaries: eclipsing
dc.subjectbinaries: spectroscopic
dc.subjectbinaries: detached
dc.subjectstars: fundamental parameters
dc.titleUpdated MS Luminosity-Radius-Temperature-Mass Relations for Solar Neighborhood Galactic Disk Stars
dc.typeConference Object

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