1 Ocak 2018 Konferans bildirisi Açık Erişim

Eker, Zeki; Bakis, Volkan; Bilir, Selcuk; Soydugan, Faruk; Steer, Ian; Soydugan, Esin; Bakis, Hicran; Alicavus, Fahri; Aslan, Gurkan; Alpsoy, Mehmet

Dublin Core

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  <dc:creator>Eker, Zeki</dc:creator>
  <dc:creator>Bakis, Volkan</dc:creator>
  <dc:creator>Bilir, Selcuk</dc:creator>
  <dc:creator>Soydugan, Faruk</dc:creator>
  <dc:creator>Steer, Ian</dc:creator>
  <dc:creator>Soydugan, Esin</dc:creator>
  <dc:creator>Bakis, Hicran</dc:creator>
  <dc:creator>Alicavus, Fahri</dc:creator>
  <dc:creator>Aslan, Gurkan</dc:creator>
  <dc:creator>Alpsoy, Mehmet</dc:creator>
  <dc:date>2018-01-01</dc:date>
  <dc:description>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.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/32963</dc:identifier>
  <dc:identifier>oai:zenodo.org:32963</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:title>Updated MS Luminosity-Radius-Temperature-Mass Relations for Solar Neighborhood Galactic Disk Stars</dc:title>
  <dc:type>info:eu-repo/semantics/conferencePaper</dc:type>
  <dc:type>publication-conferencepaper</dc:type>
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