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dc.contributor.authorHough, J.
dc.date.accessioned2009-04-22T08:24:32Z
dc.date.available2009-04-22T08:24:32Z
dc.date.issued1997
dc.identifier.citationHough , J 1997 , ' Infrared Polarimetry and the Torus ' Astrophysics and Space Science , vol. 248 , no. 1-2 , pp. 269-276 . https://doi.org/10.1023/A:1000506403087
dc.identifier.issn0004-640X
dc.identifier.otherPURE: 170784
dc.identifier.otherPURE UUID: ddaf6b2c-0a8e-4682-9301-c972440dafbb
dc.identifier.otherdspace: 2299/3261
dc.identifier.otherScopus: 0039329183
dc.identifier.urihttp://hdl.handle.net/2299/3261
dc.description“The original publication is available at www.springerlink.com”. Copyright Springer. [Full text of this article is not available in the UHRA]
dc.description.abstractPolarimetry at near-infrared wavelengths is shown to be an important tool in understanding the properties of the obscuring torus in NGC1068. We present evidence for the existence of aligned grains in the torus, which produce polarized flux through dichroism, and show how the torus itself can be observed in silhouette in polarized flux images.en
dc.language.isoeng
dc.relation.ispartofAstrophysics and Space Science
dc.titleInfrared Polarimetry and the Torusen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
rioxxterms.versionofrecordhttps://doi.org/10.1023/A:1000506403087
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue
herts.rights.accesstyperestrictedAccess


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