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dc.contributor.authorAxon, D.J.
dc.contributor.authorHough, J.
dc.contributor.authorYoung, S.
dc.contributor.authorInglis, M.D.
dc.date.accessioned2009-04-22T08:19:21Z
dc.date.available2009-04-22T08:19:21Z
dc.date.issued1994
dc.identifier.citationAxon , D J , Hough , J , Young , S & Inglis , M D 1994 , ' Hidden broad-line regions and anisotropy in AGN ' , Astrophysics and Space Science , vol. 216 , no. 1-2 , pp. 379-398 . https://doi.org/10.1007/BF00982525
dc.identifier.issn0004-640X
dc.identifier.otherdspace: 2299/3260
dc.identifier.urihttp://hdl.handle.net/2299/3260
dc.description“The original publication is available at www.springerlink.com”. Copyright Springer. DOI: 10.1007/BF00982525 [Full text of this article is not available in the UHRA]
dc.description.abstractWe discuss the recent advances made in the search for hidden broad line regions in Seyfert and Narrow Line Radio Galaxies (NLRG) using both spectropolarimetry and infrared spectroscopy/spectropolarimetry. Two important results which support the Grand Unification Theory are presented. In the first of these we report that the famous Seyfert 1 NGC 4151 has a scattered component to its broad line region, and is most likely an object where we view obliquely into its occulting torus. In the second, we show high signal to noise observations of scattered broad lines in the NLRG of 3C 234.en
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.subjectactive galactic nuclei
dc.titleHidden broad-line regions and anisotropy in AGNen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1007/BF00982525
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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