1 Ocak 2016 Dergi makalesi Açık Erişim

Budding, E.; Puskullu, C.; Rhodes, M. D.; Demircan, O.; Erdem, A.

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  "@context": "https://schema.org/", 
  "@id": 57773, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "name": "Budding, E."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Univ Canakkale, TR-17020 Canakkale, Turkey", 
      "name": "Puskullu, C."
    }, 
    {
      "@type": "Person", 
      "affiliation": "BYU, Provo, UT USA", 
      "name": "Rhodes, M. D."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Univ Canakkale, TR-17020 Canakkale, Turkey", 
      "name": "Demircan, O."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Univ Canakkale, TR-17020 Canakkale, Turkey", 
      "name": "Erdem, A."
    }
  ], 
  "datePublished": "2016-01-01", 
  "description": "We have applied the graphical user interfaced close binary system analysis program WINFITTER to an intensive study of Kepler-91 using all the available photometry from the NASA Exoplanet Archive (NEA) at the Caltech website: http://exoplanetarchive.ipac.caltech.edu. Our fitting function for the tidal distortion derives from the relevant Radau equation and includes terms up to the fifth power of the fractional radius. This results in a systematic improvement in the mass ratio estimation over that of Lillo-Box et al. (Astron. Astrophys. 562:A109, 2014a) and our derived value for the mass ratio is in close agreement with that inferred from recent high-resolution spectroscopic data.", 
  "headline": "Analysis of the exoplanet containing system Kepler-91", 
  "identifier": 57773, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Analysis of the exoplanet containing system Kepler-91", 
  "url": "https://aperta.ulakbim.gov.tr/record/57773"
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