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dc.contributor.authorEfstathiou, A.
dc.contributor.authorHough, J.
dc.contributor.authorMcCall, A.
dc.contributor.authorYoung, S.
dc.date.accessioned2008-02-01T11:46:31Z
dc.date.available2008-02-01T11:46:31Z
dc.date.issued1996
dc.identifier.citationEfstathiou , A , Hough , J , McCall , A & Young , S 1996 , A Model for the Infrared Polarization of NGC 1068 . in In: Polarimetry of the interstellar medium. ASP Conference Series 97 . Astronomical Society of the Pacific , pp. 602-6 .
dc.identifier.isbn1-886733-18-X
dc.identifier.otherdspace: 2299/1543
dc.identifier.urihttp://hdl.handle.net/2299/1543
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present a method for calculating the polarization due to absorption and emission by aligned grains distributed in a disk or a torus. The temperature distribution in the torus is calculated self-consistently with the axially symmetric radiative transfer code of Efstathiou & Rowan-Robinson (1990, 1995). The polarization patterns predicted for models that provide good fits to the spectral energy distributions of Active Galactic Nuclei (AGN) show a flip in position angle in the infrared. This effect has already been observed in the case of NGC 1068. We show that the model of Efstathiou et al. (1995) for the torus in NGC 1068 is consistent with the observed polarization pattern.en
dc.format.extent442702
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Polarimetry of the interstellar medium. ASP Conference Series 97
dc.titleA Model for the Infrared Polarization of NGC 1068en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.contributor.institutionScience & Technology Research Institute
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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