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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.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.otherPURE: 152290
dc.identifier.otherPURE UUID: d7169a7f-be3d-44fa-9141-990845217c6a
dc.identifier.otherdspace: 2299/3236
dc.descriptionOriginal article can be found via: 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.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
rioxxterms.typeJournal Article/Review

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