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Spectropolarimetry of the 3.4 micron feature in the diffuse ISM toward the galactic center quintuplet cluster

dc.contributor.authorChiar, J.E.
dc.contributor.authorAdamson, A.J.
dc.contributor.authorWhittet, D.C.B.
dc.contributor.authorChrysostomou, A.
dc.contributor.authorHough, J.
dc.contributor.authorKerr, T.H.
dc.contributor.authorMason, R.E.
dc.contributor.authorPoche, P.F.
dc.contributor.authorWright, G.
dc.date.accessioned2007-11-23T16:22:30Z
dc.date.available2007-11-23T16:22:30Z
dc.date.issued2006
dc.identifier.citationChiar , J E , Adamson , A J , Whittet , D C B , Chrysostomou , A , Hough , J , Kerr , T H , Mason , R E , Poche , P F & Wright , G 2006 , ' Spectropolarimetry of the 3.4 micron feature in the diffuse ISM toward the galactic center quintuplet cluster ' , The Astrophysical Journal , vol. 651 , no. 1 , pp. 268-271 .
dc.identifier.issn0004-637X
dc.identifier.otherdspace: 2299/1092
dc.identifier.urihttp://hdl.handle.net/2299/1092
dc.format.extent130154
dc.language.isoeng
dc.relation.ispartofThe Astrophysical Journal
dc.titleSpectropolarimetry of the 3.4 micron feature in the diffuse ISM toward the galactic center quintuplet clusteren
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.contributor.institutionCentre for Astrophysics Research (CAR)
dc.description.statusPeer reviewed
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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