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2002MNRAS.332L..55G - Mon. Not. R. Astron. Soc., 332, L55-L58 (2002/May-3)
Submillimetre photometry of post-asymptotic giant branch stars.
GLEDHILL T.M., BAINS I. and YATES J.A.
Abstract (from CDS):
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 850µm and we use these fluxes to estimate the envelope dust masses and, by comparison with the 100-µm IRAS fluxes, the dust emissivity index.
Abstract Copyright: 2002 Blackwell Science Ltd
Journal keyword(s): stars: AGB and post-AGB - circumstellar matter - stars: mass-loss - submillimetre
Simbad objects: 9
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