dc.contributor.author | Gledhill, T. | |
dc.contributor.author | Bains, I. | |
dc.contributor.author | Yates, J.A. | |
dc.date.accessioned | 2010-02-15T14:33:17Z | |
dc.date.available | 2010-02-15T14:33:17Z | |
dc.date.issued | 2002 | |
dc.identifier.citation | Gledhill , 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.issn | 0035-8711 | |
dc.identifier.other | dspace: 2299/4275 | |
dc.identifier.other | ORCID: /0000-0002-2859-4600/work/30779785 | |
dc.identifier.uri | http://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.abstract | Stars 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.iso | eng | |
dc.relation.ispartof | Monthly Notices of the Royal Astronomical Society | |
dc.title | Submillimetre photometry of post-asymptotic giant branch stars | en |
dc.contributor.institution | School of Physics, Engineering & Computer Science | |
dc.contributor.institution | Department of Physics, Astronomy and Mathematics | |
dc.contributor.institution | Centre for Astrophysics Research (CAR) | |
dc.description.status | Peer reviewed | |
rioxxterms.versionofrecord | 10.1046/j.1365-8711.2002.05550.x | |
rioxxterms.type | Journal Article/Review | |
herts.preservation.rarelyaccessed | true | |