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

DataCite XML

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/32963</identifier>
  <creators>
    <creator>
      <creatorName>Eker, Zeki</creatorName>
      <givenName>Zeki</givenName>
      <familyName>Eker</familyName>
      <affiliation>Akdeniz Univ, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Bakis, Volkan</creatorName>
      <givenName>Volkan</givenName>
      <familyName>Bakis</familyName>
      <affiliation>Akdeniz Univ, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Bilir, Selcuk</creatorName>
      <givenName>Selcuk</givenName>
      <familyName>Bilir</familyName>
      <affiliation>Istanbul Univ, Dept Astron &amp; Space Sci, TR-34119 Istanbul, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Soydugan, Faruk</creatorName>
      <givenName>Faruk</givenName>
      <familyName>Soydugan</familyName>
    </creator>
    <creator>
      <creatorName>Steer, Ian</creatorName>
      <givenName>Ian</givenName>
      <familyName>Steer</familyName>
      <affiliation>NASA IPAC Extragalact Database Distances, Toronto, ON M5A 4H2, Canada</affiliation>
    </creator>
    <creator>
      <creatorName>Soydugan, Esin</creatorName>
      <givenName>Esin</givenName>
      <familyName>Soydugan</familyName>
    </creator>
    <creator>
      <creatorName>Bakis, Hicran</creatorName>
      <givenName>Hicran</givenName>
      <familyName>Bakis</familyName>
      <affiliation>Akdeniz Univ, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Alicavus, Fahri</creatorName>
      <givenName>Fahri</givenName>
      <familyName>Alicavus</familyName>
    </creator>
    <creator>
      <creatorName>Aslan, Gurkan</creatorName>
      <givenName>Gurkan</givenName>
      <familyName>Aslan</familyName>
      <affiliation>Akdeniz Univ, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Alpsoy, Mehmet</creatorName>
      <givenName>Mehmet</givenName>
      <familyName>Alpsoy</familyName>
      <affiliation>Akdeniz Univ, Dept Space Sci &amp; Technol, TR-07058 Antalya, Turkey</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Updated Ms Luminosity-Radius-Temperature-Mass Relations For Solar Neighborhood Galactic Disk Stars</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2018</publicationYear>
  <dates>
    <date dateType="Issued">2018-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Conference paper</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/32963</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1063/1.5078888</relatedIdentifier>
  </relatedIdentifiers>
  <rightsList>
    <rights rightsURI="http://www.opendefinition.org/licenses/cc-by">Creative Commons Attribution</rights>
    <rights rightsURI="info:eu-repo/semantics/openAccess">Open Access</rights>
  </rightsList>
  <descriptions>
    <description descriptionType="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.</description>
  </descriptions>
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