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dc.contributor.authorChiar, J.E.
dc.contributor.authorAdamson, A.J.
dc.contributor.authorKerr, T.H.
dc.contributor.authorMason, R.E.
dc.contributor.authorWright, G.
dc.contributor.authorWhittet, D.C.B.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorHough, J.
dc.contributor.authorRoche, P.F.
dc.date.accessioned2008-02-01T11:36:26Z
dc.date.available2008-02-01T11:36:26Z
dc.date.issued2005
dc.identifier.citationChiar , J E , Adamson , A J , Kerr , T H , Mason , R E , Wright , G , Whittet , D C B , Chrysostomou , A , Hough , J & Roche , P F 2005 , Spectropolarimetry of the 3.4 m Band in the Quintuplet . in In: Astronomical Polarimetry: Current Status and Future Directions - ASP Conf Series 343 . Astronomical Society of the Pacific , pp. 352-6 .
dc.identifier.isbn978-1-58381-277-8
dc.identifier.isbn1-58381-210-5
dc.identifier.otherPURE: 179429
dc.identifier.otherPURE UUID: 5a8d3d34-189c-405d-9cff-dacee4a30fce
dc.identifier.otherdspace: 2299/1511
dc.identifier.urihttp://hdl.handle.net/2299/1511
dc.descriptionOriginal paper can be found at: http://161.58.115.79/pubs/cs/328.html--Copyright Astronomical Society of the Pacific
dc.description.abstractWe present spectropolarimetry of the 3.4?m solid hydrocarbon absorption feature arising in the ISM toward the Quintuplet member GCS3-II, permitting for the first time a comparison of the hydrocarbon and silicate polarizations in the same line of sight. The hydrocarbon band is not measurably polarized, strengthening our previous conclusion that the silicates and carbonaceous grains form distinct populations.en
dc.language.isoeng
dc.publisherAstronomical Society of the Pacific
dc.relation.ispartofIn: Astronomical Polarimetry: Current Status and Future Directions - ASP Conf Series 343
dc.titleSpectropolarimetry of the 3.4 m Band in the Quintupleten
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research
rioxxterms.typeOther
herts.preservation.rarelyaccessedtrue


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