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dc.contributor.authorMagalhaes, A.M.
dc.contributor.authorRodrigues, C.V.
dc.contributor.authorMeade, M.
dc.contributor.authorCode, A.D.
dc.contributor.authorNordsieck, K.H.
dc.contributor.authorAnderson, C.M.
dc.contributor.authorBailey, J.
dc.contributor.authorHough, J.
dc.contributor.authorWheatley, P.J.
dc.date.accessioned2008-02-01T11:46:34Z
dc.date.available2008-02-01T11:46:34Z
dc.date.issued1996
dc.identifier.citationMagalhaes , A M , Rodrigues , C V , Meade , M , Code , A D , Nordsieck , K H , Anderson , C M , Bailey , J , Hough , J & Wheatley , P J 1996 , Dust in a Hostile Environment: Interstellar Dust in the Line of Sight to HD62542 . in In: Polarimetry of the interstellar medium, ASP Conference Series 97 . Astronomical Society of the Pacific , pp. 202-6 .
dc.identifier.isbn1-886733-18-X
dc.identifier.otherPURE: 181147
dc.identifier.otherPURE UUID: adf03aae-ec59-4137-ab07-75cfe9e5d3eb
dc.identifier.otherdspace: 2299/1547
dc.identifier.urihttp://hdl.handle.net/2299/1547
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific
dc.description.abstractHD 62542 is situated in a line of sight toward a ridge of dark matter in the Gum Nebula. That region is under the influence of UV radiation and stellar winds from hot stars. We use for the first time interstellar polarization and extinction data from the ultraviolet to the infrared in order to study and quantify the influence of such an environment on the size of the dust particles.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Polarimetry of the interstellar medium, ASP Conference Series 97
dc.titleDust in a Hostile Environment: Interstellar Dust in the Line of Sight to HD62542en
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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