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dc.contributor.authorRobb, R.M.
dc.contributor.authorVincent, J.
dc.contributor.authorHenderson, H.
dc.contributor.authorGreimel, R.
dc.contributor.authorDrew, J.E.
dc.contributor.authorGonzalez-Solares, E.
dc.date.accessioned2008-12-08T15:59:28Z
dc.date.available2008-12-08T15:59:28Z
dc.date.issued2008
dc.identifier.citationRobb , R M , Vincent , J , Henderson , H , Greimel , R , Drew , J E & Gonzalez-Solares , E 2008 , ' The New Contact Binary GSC 2414-0797 ' , Information Bulletin on Variable Stars , vol. 5852 .
dc.identifier.issn1587-2440
dc.identifier.otherPURE: 148917
dc.identifier.otherPURE UUID: a080fb34-ce87-4bba-a84c-33657e80b289
dc.identifier.otherdspace: 2299/2677
dc.identifier.otherScopus: 56349169349
dc.identifier.urihttp://hdl.handle.net/2299/2677
dc.descriptionOriginal article can be found at: http://www.konkoly.hu/ibvs/
dc.description.abstractGSC 2414-0797 has a contact binary star type light curve, a 0.4 magnitude brightness variation with a period 0.3406 days.en
dc.language.isoeng
dc.relation.ispartofInformation Bulletin on Variable Stars
dc.titleThe New Contact Binary GSC 2414-0797en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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