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dc.contributor.authorPratt, GW
dc.contributor.authorHassall, BJM
dc.contributor.authorNaylor, T
dc.contributor.authorWood, JH
dc.date.accessioned2017-06-20T08:04:06Z
dc.date.issued1999-08-01
dc.description.abstractWe present a phase-resolved ROSAT HRI X-ray light curve of the dwarf nova OY Car in quiescence. The X-ray flux is eclipsed at the same time as the optical eclipse of the primary, and the region of X -ray emission is comparable in size to the white dwarf. We use subsequent optical observations to update the orbital ephemeris of the system.en_GB
dc.description.sponsorshipWe thank Jakob Engelhauser for his help with the difficult scheduling of the ROSAT observations. We acknowledge the data analysis facilities provided by the Starlink Project, which is run by CCLRC on behalf of PPARC. GWP is in receipt of a University of Central Lancashire research studentship.en_GB
dc.identifier.citationVol. 307, pp. 413 - 419en_GB
dc.identifier.doi10.1046/j.1365-8711.1999.02601.x
dc.identifier.urihttp://hdl.handle.net/10871/28098
dc.language.isoenen_GB
dc.publisherOxford University Press (OUP) / Royal Astronomical Societyen_GB
dc.relation.urlhttp://adsabs.harvard.edu/abs/1999MNRAS.307..413Pen_GB
dc.subjectaccretion, accretion discsen_GB
dc.subjectbinaries: eclipsingen_GB
dc.subjectstars: individual: OY Caren_GB
dc.subjectnovae, cataclysmic variablesen_GB
dc.subjectX-rays: starsen_GB
dc.titleAn eclipse of the X-ray flux from the dwarf nova OY Carinae in quiescenceen_GB
dc.typeArticleen_GB
dc.date.available2017-06-20T08:04:06Z
dc.identifier.issn0035-8711
dc.descriptionThis is the author accepted manuscript. The final version is available from the publisher via the DOI in this record.en_GB
dc.identifier.journalMonthly Notices of the Royal Astronomical Societyen_GB


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