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dc.contributor.authorInglis, M.D.
dc.contributor.authorBrindle, C.
dc.contributor.authorHough, J.
dc.contributor.authorYoung, S.
dc.contributor.authorAxon, D.J.
dc.contributor.authorBailey, J.
dc.contributor.authorWard, M.J.
dc.date.accessioned2009-04-21T07:48:15Z
dc.date.available2009-04-21T07:48:15Z
dc.date.issued1993
dc.identifier.citationInglis , M D , Brindle , C , Hough , J , Young , S , Axon , D J , Bailey , J & Ward , M J 1993 , ' Evidence for an Obscured Broadline Region in the Early Type Radio Galaxy IC5063 ' , Monthly Notices of the Royal Astronomical Society , vol. 263 , no. 4 , pp. 895-902 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 152290
dc.identifier.otherPURE UUID: d7169a7f-be3d-44fa-9141-990845217c6a
dc.identifier.otherdspace: 2299/3236
dc.identifier.urihttp://hdl.handle.net/2299/3236
dc.descriptionOriginal article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractWe report the detection of strong, broad Hα emission seen in polarized flux from the early-type radio galaxy IC 5063. This suggests that the galaxy has a broad-line region which is obscured from our direct view, with the broad-line radiation being scattered into our line of sight by scatterers outside the obscuring regions. A model has been developed to estimate the dilution by starlight of the intrinsic polarization, and to correct for interstellar polarization. The FWHM of the broad Hα is 3400 km s^-1^, well within the range covered by typical Seyfert 1 galaxies.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleEvidence for an Obscured Broadline Region in the Early Type Radio Galaxy IC5063en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1993
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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