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dc.contributor.authorBailey, J.
dc.contributor.authorHough, J.
dc.contributor.authorSchwarzenbergczerny, A.
dc.contributor.authorGatley, I.
dc.contributor.authorJameson, R.F.
dc.contributor.authorHanes, D.A.
dc.date.accessioned2009-04-22T09:52:53Z
dc.date.available2009-04-22T09:52:53Z
dc.date.issued1981
dc.identifier.citationBailey , J , Hough , J , Schwarzenbergczerny , A , Gatley , I , Jameson , R F & Hanes , D A 1981 , ' The X-ray cataclysmic variable 1E0643.0 −1648 ' , Nature , vol. 293 , no. 5829 , pp. 204-206 . https://doi.org/10.1038/293204a0
dc.identifier.issn0028-0836
dc.identifier.otherdspace: 2299/3265
dc.identifier.urihttp://hdl.handle.net/2299/3265
dc.descriptionOriginal article can be found at: http://www.nature.com/nature/index.html Copyright Nature Publishing Group. DOI: 10.1038/293204a0 [Full text of this article is not available in the UHRA]
dc.description.abstractWe have used a new simultaneous IR/optical high-speed photometer on the UK IR telescope to study the recently discovered X-ray cataclysmic variable 1E0643.0−1648 (refs 1, 2). The light curve of this object obtained by the American Association of Variable Star Observers (AAVSO) (T. Chlebowski, personal communication) has shown it to be a dwarf nova with a recurrence time scale of 15 days. We report here that our photometry, obtained during the decline from an outburst, shows slow flickering, with the optical and IR light curves correlated with no delay. We have also obtained moderate resolution spectra of the star using the Anglo−Australian telescope.en
dc.language.isoeng
dc.relation.ispartofNature
dc.titleThe X-ray cataclysmic variable 1E0643.0 −1648en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1038/293204a0
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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