1 Ocak 2016 Dergi makalesi Açık Erişim

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

Dublin Core

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  <dc:creator>Budding, E.</dc:creator>
  <dc:creator>Puskullu, C.</dc:creator>
  <dc:creator>Rhodes, M. D.</dc:creator>
  <dc:creator>Demircan, O.</dc:creator>
  <dc:creator>Erdem, A.</dc:creator>
  <dc:date>2016-01-01</dc:date>
  <dc: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.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/57773</dc:identifier>
  <dc:identifier>oai:zenodo.org:57773</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>ASTROPHYSICS AND SPACE SCIENCE 361(1)</dc:source>
  <dc:title>Analysis of the exoplanet containing system Kepler-91</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
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