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dc.contributor.authorAitken, D.
dc.contributor.authorHough, J.
dc.contributor.authorRoche, P.F.
dc.contributor.authorSmith, C.H.
dc.contributor.authorWright, C.M.
dc.date.accessioned2010-02-18T09:15:38Z
dc.date.available2010-02-18T09:15:38Z
dc.date.issued2004
dc.identifier.citationAitken , D , Hough , J , Roche , P F , Smith , C H & Wright , C M 2004 , ' Mid-infrared polarimetry and magnetic fields : an observing strategy ' , Monthly Notices of the Royal Astronomical Society , vol. 348 , no. 1 , pp. 279-284 . https://doi.org/10.1111/j.1365-2966.2004.07365.x
dc.identifier.issn0035-8711
dc.identifier.otherdspace: 2299/4283
dc.identifier.urihttp://hdl.handle.net/2299/4283
dc.description‘The definitive version is available at www.blackwell-synergy.com '. Copyright Blackwell Publishing. DOI: 10.1111/j.1365-2966.2004.07365.x [Full text of this article is not available in the UHRA]
dc.description.abstractLinear polarimetry in the mid-infrared can be used to obtain magnetic field directions in astronomical sources. However, since the polarization can arise from emission and/or absorption from aligned grains, care is needed to plan observations so that enough information is obtained to identify and separate the components of polarization. Procedures for doing this from spectropolarimetry, and from polarimetric imaging at a minimum of two wavebands and making an appropriate filter choice, are presented here, together with an example.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleMid-infrared polarimetry and magnetic fields : an observing strategyen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionScience & Technology Research Institute
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.versionofrecord10.1111/j.1365-2966.2004.07365.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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