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.

JSON-LD (schema.org)

{
  "@context": "https://schema.org/", 
  "@id": 98567, 
  "@type": "ScholarlyArticle", 
  "creator": [
    {
      "@type": "Person", 
      "affiliation": "Kazan Volga Reg Fed Univ, Kazan 420008, Russia", 
      "name": "Sklyanov, A. S."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Crimean Astrophys Observ, Nauchny 098409, Russia", 
      "name": "Pavlenko, E. P."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Crimean Astrophys Observ, Nauchny 098409, Russia", 
      "name": "Antonyuk, O. I."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Crimean Astrophys Observ, Nauchny 098409, Russia", 
      "name": "Antonyuk, K. A."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Crimean Astrophys Observ, Nauchny 098409, Russia", 
      "name": "Sosnovsky, A. A."
    }, 
    {
      "@type": "Person", 
      "name": "Galeev, A. I."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Crimean Astrophys Observ, Nauchny 098409, Russia", 
      "name": "Pit', N. V."
    }, 
    {
      "@type": "Person", 
      "affiliation": "Crimean Astrophys Observ, Nauchny 098409, Russia", 
      "name": "Babina, Yu. V."
    }
  ], 
  "datePublished": "2016-01-01", 
  "description": "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).", 
  "headline": "Superhump evolution of WZ Sge-type dwarf nova ASASSN-14cv at rebrightening stage", 
  "identifier": 98567, 
  "image": "https://aperta.ulakbim.gov.tr/static/img/logo/aperta_logo_with_icon.svg", 
  "license": "http://www.opendefinition.org/licenses/cc-by", 
  "name": "Superhump evolution of WZ Sge-type dwarf nova ASASSN-14cv at rebrightening stage", 
  "url": "https://aperta.ulakbim.gov.tr/record/98567"
}