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dc.contributor.authorGledhill, T.
dc.contributor.authorBains, I.
dc.contributor.authorYates, J.A.
dc.date.accessioned2010-02-15T14:33:17Z
dc.date.available2010-02-15T14:33:17Z
dc.date.issued2002
dc.identifier.citationGledhill , T , Bains , I & Yates , J A 2002 , ' Submillimetre photometry of post-asymptotic giant branch stars ' , Monthly Notices of the Royal Astronomical Society , vol. 332 , no. 3 , pp. L55-L58 . https://doi.org/10.1046/j.1365-8711.2002.05550.x
dc.identifier.issn0035-8711
dc.identifier.otherPURE: 175914
dc.identifier.otherPURE UUID: 51aee0e2-0e51-468e-b765-2622ecc9f2d9
dc.identifier.otherdspace: 2299/4275
dc.identifier.otherScopus: 0042692790
dc.identifier.otherORCID: /0000-0002-2859-4600/work/30779785
dc.identifier.urihttp://hdl.handle.net/2299/4275
dc.description‘The definitive version is available at www.blackwell-synergy.com '. Copyright Royal Astronomical Society. DOI: 10.1046/j.1365-8711.2002.05550.x [Full text of this article is not available in the UHRA]
dc.description.abstractStars in the post-asymptotic giant branch (post-AGB) phase of evolution are surrounded by detached circumstellar envelopes containing dust which emits thermally in the mid- and far-infrared. Here we present 850-μm SCUBA photometry of nine candidate post-AGB stars. All targets are detected at 850 μm and we use these fluxes to estimate the envelope dust masses and, by comparison with the 100-μm IRAS fluxes, the dust emissivity index.en
dc.language.isoeng
dc.relation.ispartofMonthly Notices of the Royal Astronomical Society
dc.titleSubmillimetre photometry of post-asymptotic giant branch starsen
dc.contributor.institutionSchool of Physics, Astronomy and Mathematics
dc.description.statusPeer reviewed
rioxxterms.versionofrecordhttps://doi.org/10.1046/j.1365-8711.2002.05550.x
rioxxterms.typeJournal Article/Review
herts.preservation.rarelyaccessedtrue


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