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dc.contributor.authorVoloshina, I.
dc.contributor.authorMetlov, V.
dc.date.accessioned2023-01-18T14:26:13Z
dc.date.available2023-01-18T14:26:13Z
dc.date.issued2015
dc.identifier.citationActa Polytechnica. 2015, vol. 2, no. 1, p. 161-164.
dc.identifier.issn1210-2709 (print)
dc.identifier.issn1805-2363 (online)
dc.identifier.urihttp://hdl.handle.net/10467/105775
dc.description.abstractIn this work we present time-resolved photometry of several poorly-studied dwarf novae during recent superoutbursts. Observations were made with a CCD, mounted on 50- and 60-cm telescopes of the Sternberg Astronomical Institute in Crimea in April - May and October 2012 and June - July 2013. Superhumps were detected in light curves of all the dwarf novae. The amplitudes and periods of detected light variations were calculated. Superhumps evolution was also followed up for all systems and classification is improved.en
dc.format.mimetypeapplication/pdf
dc.language.isoeng
dc.publisherČeské vysoké učení technické v Prazecs
dc.publisherCzech Technical University in Pragueen
dc.relation.ispartofseriesActa Polytechnica
dc.relation.urihttps://ojs.cvut.cz/ojs/index.php/APP/article/view/2874
dc.rightsCreative Commons Attribution 4.0 International Licenseen
dc.rights.urihttp://creativecommons.org/licenses/by/4.0/
dc.titleStudy of Photometric Variability of Selected SU UMa Dwarf Novae
dc.typearticleen
dc.date.updated2023-01-18T14:26:13Z
dc.identifier.doi10.14311/APP.2015.02.0161
dc.rights.accessopenAccess
dc.type.statusPeer-reviewed
dc.type.versionpublishedVersion


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Creative Commons Attribution 4.0 International License
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