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Eker, Zeki; Bakis, Volkan; Bilir, Selcuk; Soydugan, Faruk; Steer, Ian; Soydugan, Esin; Bakis, Hicran; Alicavus, Fahri; Aslan, Gurkan; Alpsoy, Mehmet
{ "DOI": "10.1063/1.5078888", "abstract": "Conventional 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.", "author": [ { "family": "Eker", "given": " Zeki" }, { "family": "Bakis", "given": " Volkan" }, { "family": "Bilir", "given": " Selcuk" }, { "family": "Soydugan", "given": " Faruk" }, { "family": "Steer", "given": " Ian" }, { "family": "Soydugan", "given": " Esin" }, { "family": "Bakis", "given": " Hicran" }, { "family": "Alicavus", "given": " Fahri" }, { "family": "Aslan", "given": " Gurkan" }, { "family": "Alpsoy", "given": " Mehmet" } ], "id": "32963", "issued": { "date-parts": [ [ 2018, 1, 1 ] ] }, "title": "Updated MS Luminosity-Radius-Temperature-Mass Relations for Solar Neighborhood Galactic Disk Stars", "type": "paper-conference" }
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