1 Ocak 2013 Dergi makalesi Açık Erişim

Cakirli, Omur

Dublin Core

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  <dc:creator>Cakirli, Omur</dc:creator>
  <dc:date>2013-01-01</dc:date>
  <dc:description>The multi-color photometric and spectroscopic(1) observations of the newly discovered eclipsing binary NSVS 07394765 were obtained. The resultant light and radial velocities were analysed and the global parameters of the system: T-1 = 3300 K; T-2 = 3106 K; M-1 = 0.36 M-circle dot,; M-2 = 0.18 M-circle dot; R-1 = 0.46 R-circle dot; R-2 = 0.50 R-circle dot; L-1 = 0.030 L-circle dot; L-2 = 0.026 L-circle dot; i = 89.2 degrees; a = 5.97 R-circle dot; d = 28 pc. The chromospheric activity of its components is revealed by strong emission in the H alpha line and observed flares. Empirical relations for mass-radius and mass-temperature are derived on the basis of the parameters of known binaries with low-mass dM components. (C) 2012 Elsevier B.V. All rights reserved.</dc:description>
  <dc:identifier>https://aperta.ulakbim.gov.trrecord/16111</dc:identifier>
  <dc:identifier>oai:zenodo.org:16111</dc:identifier>
  <dc:rights>info:eu-repo/semantics/openAccess</dc:rights>
  <dc:rights>http://www.opendefinition.org/licenses/cc-by</dc:rights>
  <dc:source>NEW ASTRONOMY 22 15-21</dc:source>
  <dc:title>NSVS 07394765: A new low-mass eclipsing binary below 0.6 M-circle dot</dc:title>
  <dc:type>info:eu-repo/semantics/article</dc:type>
  <dc:type>publication-article</dc:type>
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