1 Ocak 2016 Dergi makalesi Açık Erişim

Sklyanov, A. S.; Pavlenko, E. P.; Antonyuk, O. I.; Antonyuk, K. A.; Sosnovsky, A. A.; Galeev, A. I.; Pit', N. V.; Babina, Yu. V.

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  <identifier identifierType="URL">https://aperta.ulakbim.gov.tr/record/98567</identifier>
  <creators>
    <creator>
      <creatorName>Sklyanov, A. S.</creatorName>
      <givenName>A. S.</givenName>
      <familyName>Sklyanov</familyName>
      <affiliation>Kazan Volga Reg Fed Univ, Kazan 420008, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Pavlenko, E. P.</creatorName>
      <givenName>E. P.</givenName>
      <familyName>Pavlenko</familyName>
      <affiliation>Crimean Astrophys Observ, Nauchny 098409, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Antonyuk, O. I.</creatorName>
      <givenName>O. I.</givenName>
      <familyName>Antonyuk</familyName>
      <affiliation>Crimean Astrophys Observ, Nauchny 098409, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Antonyuk, K. A.</creatorName>
      <givenName>K. A.</givenName>
      <familyName>Antonyuk</familyName>
      <affiliation>Crimean Astrophys Observ, Nauchny 098409, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Sosnovsky, A. A.</creatorName>
      <givenName>A. A.</givenName>
      <familyName>Sosnovsky</familyName>
      <affiliation>Crimean Astrophys Observ, Nauchny 098409, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Galeev, A. I.</creatorName>
      <givenName>A. I.</givenName>
      <familyName>Galeev</familyName>
    </creator>
    <creator>
      <creatorName>Pit', N. V.</creatorName>
      <givenName>N. V.</givenName>
      <familyName>Pit'</familyName>
      <affiliation>Crimean Astrophys Observ, Nauchny 098409, Russia</affiliation>
    </creator>
    <creator>
      <creatorName>Babina, Yu. V.</creatorName>
      <givenName>Yu. V.</givenName>
      <familyName>Babina</familyName>
      <affiliation>Crimean Astrophys Observ, Nauchny 098409, Russia</affiliation>
    </creator>
  </creators>
  <titles>
    <title>Superhump Evolution Of Wz Sge-Type Dwarf Nova Asassn-14Cv At Rebrightening Stage</title>
  </titles>
  <publisher>Aperta</publisher>
  <publicationYear>2016</publicationYear>
  <dates>
    <date dateType="Issued">2016-01-01</date>
  </dates>
  <resourceType resourceTypeGeneral="Text">Journal article</resourceType>
  <alternateIdentifiers>
    <alternateIdentifier alternateIdentifierType="url">https://aperta.ulakbim.gov.tr/record/98567</alternateIdentifier>
  </alternateIdentifiers>
  <relatedIdentifiers>
    <relatedIdentifier relatedIdentifierType="DOI" relationType="IsIdenticalTo">10.1134/S1990341316030044</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 report the results of observations of a WZ Sge-type dwarf nova ASASSN-14cv, acquired in 2014 and covering the end of a superoutburst and a rebrightening stage. We detected 8 rebrightenings of this star. Based on the light curve profiles of the rebrightenings, we conclude on the existence of both the "inside-out" and "outside-in" outbursts. During the entire course of the rebrightening stage, a brightness variability with the mean period of P = 0.(d)06042(8) was detected, which was identified as a superhump period during the stage B of the superoutburst. The character of the registered superhump evolution can be either described by a parabolic approximation with the negative P (dot) = -1.1 x 10(-5), or by an approximation with 2 linear areas with the corresponding periods of 0.(d)06074(3) and 0.(d)06046(9).</description>
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