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Sklyanov, A. S.; Pavlenko, E. P.; Antonyuk, O. I.; Antonyuk, K. A.; Sosnovsky, A. A.; Galeev, A. I.; Pit', N. V.; Babina, Yu. V.
<?xml version='1.0' encoding='utf-8'?> <resource xmlns:xsi="http://www.w3.org/2001/XMLSchema-instance" xmlns="http://datacite.org/schema/kernel-4" xsi:schemaLocation="http://datacite.org/schema/kernel-4 http://schema.datacite.org/meta/kernel-4.1/metadata.xsd"> <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> </descriptions> </resource>
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