1 Ocak 2019 Dergi makalesi Açık Erişim

Cokluk, K. A.; Kocak, D.; Icli, T.; Karakose, S.; Ustundag, S.; Yakut, K.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/68921</identifier>
  <creators>
    <creator>
      <creatorName>Cokluk, K. A.</creatorName>
      <givenName>K. A.</givenName>
      <familyName>Cokluk</familyName>
      <affiliation>Univ Ege, Dept Astron &amp; Space Sci, TR-35100 Izmir, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Kocak, D.</creatorName>
      <givenName>D.</givenName>
      <familyName>Kocak</familyName>
      <affiliation>Univ Ege, Dept Astron &amp; Space Sci, TR-35100 Izmir, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Icli, T.</creatorName>
      <givenName>T.</givenName>
      <familyName>Icli</familyName>
      <affiliation>Univ Ege, Dept Astron &amp; Space Sci, TR-35100 Izmir, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Karakose, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Karakose</familyName>
      <affiliation>Univ Ege, Dept Astron &amp; Space Sci, TR-35100 Izmir, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Ustundag, S.</creatorName>
      <givenName>S.</givenName>
      <familyName>Ustundag</familyName>
      <affiliation>Univ Ege, Dept Astron &amp; Space Sci, TR-35100 Izmir, Turkey</affiliation>
    </creator>
    <creator>
      <creatorName>Yakut, K.</creatorName>
      <givenName>K.</givenName>
      <familyName>Yakut</familyName>
      <affiliation>Univ Ege, Dept Astron &amp; Space Sci, TR-35100 Izmir, Turkey</affiliation>
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  <titles>
    <title>Absolute Properties Of Ru Cnc Revisited: An Active Rs Cvn-Type Eclipsing Binary With Red Giant Branch And Main-Sequence Components</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2019</publicationYear>
  <dates>
    <date dateType="Issued">2019-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/68921</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1093/mnras/stz2051</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">We present observations and analysis of an RS CVn-type double-lined eclipsing binary system, RU Cnc. The system has been observed for over a century. High-quality long-cadence observations, newly obtained from the Kepler K2 C5 and C18 campaigns, and two radial velocity curves were combined and analysed simultaneously, assuming a multispot model. The masses, radii and luminosities of the component stars have been precisely obtained as , , , , and, with a separation of . The distance of the system is determined to be pc, which is consistent with the Gaia Data Release 2 result. Long-term detailed period variation analysis of the system indicates a period decrease of 7.9x10(-7) d yr(-1). The results suggest that the cooler component is on the red giant branch (RGB) and the hotter component is still on the main sequence.</description>
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