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dc.contributor.authorMessinger, D.W.
dc.contributor.authorRoberge, W.G.
dc.contributor.authorWhittet, D.C.B.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorHough, J.
dc.date.accessioned2008-02-01T11:36:28Z
dc.date.available2008-02-01T11:36:28Z
dc.date.issued1996
dc.identifier.citationMessinger , D W , Roberge , W G , Whittet , D C B , Chrysostomou , A & Hough , J 1996 , Modeling New Spectropolarimetry Data for the BN Object . in In: Polarimetry of the interstellar medium. ASP Conference Series 97 . Astronomical Society of the Pacific , pp. 249-253 .
dc.identifier.isbn1-886733-18-X
dc.identifier.otherPURE: 142699
dc.identifier.otherPURE UUID: befbabc1-7265-40d3-b58e-4df91b1b00d2
dc.identifier.otherdspace: 2299/1513
dc.identifier.urihttp://hdl.handle.net/2299/1513
dc.descriptionOriginal paper can be found at: http://www.astrosociety.org/pubs/cs/070-112.html--Copyright Astronomical Society of the Pacific
dc.description.abstractNew spectropolarimetry data taken for the BN object include many previously unobserved features. Among these are a possible polarization reversal at the short wavelength end of the ice feature and a rotation in the position angle across this feature. These are modeled using the dipole approximation to calculate the properties of the grain ensemble and a simple radiative transfer model of the Stokes parameters to determine the observed polarization. By matching these models to the new and better data, we will better constrain the grain properties and morphology along this line of sight than has previously been done.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Polarimetry of the interstellar medium. ASP Conference Series 97
dc.rightsOpen
dc.titleModeling New Spectropolarimetry Data for the BN Objecten
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.relation.schoolSchool of Physics, Astronomy and Mathematics
dcterms.dateAccepted1996
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue
herts.rights.accesstypeOpen


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