Please use this identifier to cite or link to this item: http://hdl.handle.net/2381/26288
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dc.contributor.authorByckling, K.-
dc.contributor.authorOsborne, J. P.-
dc.contributor.authorWynn, G. A.-
dc.contributor.authorBeardmore, A.-
dc.contributor.authorBraito, V.-
dc.contributor.authorWest, R. G.-
dc.contributor.authorWheatley, P. J.-
dc.contributor.authorMukai, K.-
dc.date.accessioned2012-10-24T09:21:31Z-
dc.date.available2012-10-24T09:21:31Z-
dc.date.issued2009-11-01-
dc.identifier.citationMonthly Notices of the Royal Astronomical Society, 2009, 399 (3), pp. 1576-1586-
dc.identifier.issn0035-8711-
dc.identifier.urihttp://hdl.handle.net/2381/26288-
dc.identifier.urihttp://mnras.oxfordjournals.org/content/399/3/1576-
dc.description.abstractThe second known outburst of the WZ Sge type dwarf nova GW Lib was observed in 2007 April. We have obtained unique multiwavelength data of this outburst which lasted ∼26 days. The American Association of Variable Star Observers (AAVSO) recorded the outburst in the optical, which was also monitored by Wide Angle Search for Planets, with a peak V magnitude of ∼8. The outburst was followed in the ultraviolet and X-ray wavelengths by the Swift ultraviolet/optical and X-ray telescopes. The X-ray flux at optical maximum was found to be three orders of magnitude above the pre-outburst quiescent level, whereas X-rays are normally suppressed during dwarf nova outbursts. A distinct supersoft X-ray component was also detected at optical maximum, which probably arises from an optically thick boundary layer. Follow-up Swift observations taken 1 and 2 years after the outburst show that the post-outburst quiescent X-ray flux remains an order of magnitude higher than the pre-outburst flux. The long interoutburst time-scale of GW Lib with no observed normal outbursts support the idea that the inner disc in GW Lib is evacuated or the disc viscosity is very low.-
dc.publisherOxford University Press (OUP)-
dc.rightsThis article has been accepted for publication in Monthly Notices of the Royal Astronomical Society ©: 2009 the authors. Published by Oxford University Press on behalf of the Royal Astronomical Society. All rights reserved. Deposited with reference to the publisher’s archiving policy available on the SHERPA/RoMEO website.-
dc.sourceScopus-
dc.source.urihttp://www.scopus.com/home.url-
dc.titleSwift observations of GW Lib: A unique insight into a rare outburst-
dc.typeJournal Article-
dc.identifier.doi10.1111/j.1365-2966.2009.15378.x-
dc.identifier.eissn1365-2966-
dc.description.statusPeer-reviewed-
dc.description.versionPublisher Version-
dc.description.irispid9059-
Appears in Collections:Published Articles, Dept. of Physics and Astronomy

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