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dc.contributor.authorHough, J.
dc.contributor.authorBailey, J.
dc.contributor.authorRouse, M.F.
dc.contributor.authorWhittet, D.C.B.
dc.date.accessioned2009-04-20T09:15:20Z
dc.date.available2009-04-20T09:15:20Z
dc.date.issued1987
dc.identifier.citationHough , J , Bailey , J , Rouse , M F & Whittet , D C B 1987 , ' Interstellar polarization in the dust lane of Centaurus A (NGC 5128) ' , Monthly Notices of the Royal Astronomical Society , vol. 227 , no. 1 , pp. 1-5 .
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 152811
dc.identifier.otherPURE UUID: 0df0bd7c-b216-4012-b4bc-a6f59c8f2e24
dc.identifier.otherdspace: 2299/3209
dc.identifier.urihttp://hdl.handle.net/2299/3209
dc.descriptionOriginal article can be found via: http://cdsads.u-strasbg.fr/ Copyright Royal Astronomical Society [Full text of this article is not available in the UHRA]
dc.description.abstractOptical and infrared linear polarization measurements of the Type 1 supernova 1986G in Centaurus A are used to determine the wavelength dependence of polarization produced by transmission of radiation through the dust lane of the galaxy. The observations are consistent with the standard form of interstellar polarization used in our Galaxy with values of Pmax= (5.16±0.04) per cent and λmax= (0.43±0.01)μm, with foreground material in our Galaxy contributing no more than ≡0.5 per cent to the observed polarization. The efficiency of alignment of the grains in Cen A is smaller than found in the Milky Way.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleInterstellar polarization in the dust lane of Centaurus A (NGC 5128)en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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