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dc.contributor.authorZejda, Miloslav
dc.contributor.authorMikulášek, Zdeněk
dc.contributor.authorZhu, L.-Y.
dc.contributor.authorQian, Sheng-Bang
dc.contributor.authorLiška, Jiří
dc.contributor.authorJaník, Jan
dc.date.accessioned2015-01-19T14:33:41Z
dc.date.available2015-01-19T14:33:41Z
dc.date.issued2014
dc.identifier.citationContributions of the Astronomical Observatory Skalnaté Pleso. 2014, vol. 43, no. 3, p. 462-464.cs
dc.identifier.issn1335-1842
dc.identifier.issn1336-0337
dc.identifier.urihttp://hdl.handle.net/10084/106319
dc.description.abstractV1010 Oph is a relatively bright near contact binary. We present a new study including four-colour photometry and a model of the system. The uniqueness of our study is in the using of only a centimetre-class telescope with a CCD camera. We show that such small, cheap equipment seems to be very helpful in the investigation of bright variable stars.cs
dc.language.isoencs
dc.publisherAstronomický ústav Slovenskej akadémie viedcs
dc.relation.ispartofseriesContributions of the Astronomical Observatory Skalnaté Plesocs
dc.relation.urihttp://www.ta3.sk/caosp/Eedition/FullTexts/vol43no3/pp462-464.pdfcs
dc.titleV1010 Oph investigated by a cm-class telescopecs
dc.typearticlecs
dc.type.statusPeer-reviewedcs
dc.description.sourceWeb of Sciencecs
dc.description.volume43cs
dc.description.issue3cs
dc.description.lastpage464cs
dc.description.firstpage462cs
dc.identifier.wos000338483100066


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