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

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{
  "@context": "https://schema.org/", 
  "@id": 32963, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "affiliation": "Akdeniz Univ, Dept Space Sci & Technol, TR-07058 Antalya, Turkey", 
      "name": "Eker, Zeki"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Akdeniz Univ, Dept Space Sci & Technol, TR-07058 Antalya, Turkey", 
      "name": "Bakis, Volkan"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Istanbul Univ, Dept Astron & Space Sci, TR-34119 Istanbul, Turkey", 
      "name": "Bilir, Selcuk"
    }, 
    {
      "@type": "Person", 
      "name": "Soydugan, Faruk"
    }, 
    {
      "@type": "Person", 
      "affiliation": "NASA IPAC Extragalact Database Distances, Toronto, ON M5A 4H2, Canada", 
      "name": "Steer, Ian"
    }, 
    {
      "@type": "Person", 
      "name": "Soydugan, Esin"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Akdeniz Univ, Dept Space Sci & Technol, TR-07058 Antalya, Turkey", 
      "name": "Bakis, Hicran"
    }, 
    {
      "@type": "Person", 
      "name": "Alicavus, Fahri"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Akdeniz Univ, Dept Space Sci & Technol, TR-07058 Antalya, Turkey", 
      "name": "Aslan, Gurkan"
    }, 
    {
      "@type": "Person", 
      "affiliation": "Akdeniz Univ, Dept Space Sci & Technol, TR-07058 Antalya, Turkey", 
      "name": "Alpsoy, Mehmet"
    }
  ], 
  "datePublished": "2018-01-01", 
  "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.", 
  "headline": "Updated MS Luminosity-Radius-Temperature-Mass Relations for Solar Neighborhood Galactic Disk Stars", 
  "identifier": 32963, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Updated MS Luminosity-Radius-Temperature-Mass Relations for Solar Neighborhood Galactic Disk Stars", 
  "url": "https://aperta.ulakbim.gov.tr/record/32963"
}