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dc.contributor.authorYoung, S.
dc.contributor.authorHough, J.
dc.contributor.authorBailey, J.
dc.contributor.authorAxon, D.J.
dc.contributor.authorWard, M.J.
dc.date.accessioned2009-04-17T13:33:25Z
dc.date.available2009-04-17T13:33:25Z
dc.date.issued1993
dc.identifier.citationYoung , S , Hough , J , Bailey , J , Axon , D J & Ward , M J 1993 , ' Spectropolarimetry of the ultraluminous infrared galaxy IRAS 110548-1131 ' , Monthly Notices of the Royal Astronomical Society , vol. 260 , no. 1 , pp. L1-L3 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 152353
dc.identifier.otherPURE UUID: 34ea58f4-9003-4a41-b044-9edbabd7dc2d
dc.identifier.otherdspace: 2299/3196
dc.identifier.urihttp://hdl.handle.net/2299/3196
dc.descriptionCopyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractFrom spectropolarimetric observations of the galaxy IRAS 110548-1131 we report very strong, broad H-alpha emission (FWHM 7600 km/s) in the polarized flux spectrum. This suggests that IRAS 110548-1131 has an obscured broad-line region, the radiation of which is scattered into our line of sight by scatterers outside the obscured region.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleSpectropolarimetry of the ultraluminous infrared galaxy IRAS 110548-1131en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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