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dc.contributor.authorAlexander, D.M.
dc.contributor.authorYoung, S.
dc.contributor.authorHough, J.
dc.date.accessioned2009-04-16T10:31:12Z
dc.date.available2009-04-16T10:31:12Z
dc.date.issued1999
dc.identifier.citationAlexander , D M , Young , S & Hough , J 1999 , ' Polarized broad HeI and Paschen lines in NGC 1068 ' , Monthly Notices of the Royal Astronomical Society , vol. 304 , no. 1 , pp. L1-L4 . https://doi.org/10.1046/j.1365-8711.1999.02417.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 160564
dc.identifier.otherPURE UUID: 2d3b8a90-f023-41ca-b028-d3c44e7be43d
dc.identifier.otherdspace: 2299/3186
dc.identifier.otherScopus: 0039768954
dc.identifier.urihttp://hdl.handle.net/2299/3186
dc.description‘The definitive version is available at www3.interscience.wiley.com '. Copyright Blackwell Publishing / Royal Astronomical Society. DOI: 10.1046/j.1365-8711.1999.02417.x [Full text of this article is not available in the UHRA]
dc.description.abstractWe present J-band spectropolarimetry of NGC 1068. We observe polarized broad Pa β and, for the first time, polarized broad Pa γ and HeI. Assuming electron scattering as the polarization mechanism, the polarized broad lines suffer little or no extinction. All the polarized broad lines are redshifted with respect to the narrow lines, attributed to an outflow velocity for the scatterers of 900 ± 200 km s-1.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titlePolarized broad HeI and Paschen lines in NGC 1068en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1046/j.1365-8711.1999.02417.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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