2002MNRAS.332L..55G

Query : 2002MNRAS.332L..55G

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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Number of rows : 9
N Identifier Otype ICRS (J2000)
RA 		ICRS (J2000)
DEC 		Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2026 		#notes
1 HD 161796 pA* 17 44 55.4694563472 +50 02 39.482823336 8.00 7.68 7.21 6.77 6.51 F3Ib 335 0
2 HD 335675 pA* 18 11 30.6621530616 +27 05 15.637762608   11.52 10.55     F3Ib 119 0
3 HD 179821 pA* 19 13 58.6082398776 +00 07 31.935181836 10.81 9.694 8.19     G4_0-Ia 247 0
4 HD 331319 pA* 19 49 29.5618298904 +31 27 16.248771432 10.4 9.91 9.32 9.24   F3Ibe 99 0
5 HD 187885 pA* 19 52 52.7033593752 -17 01 50.289441096   9.25 8.68 8.32   F2/6Ia 185 0
6 IRAS 20000+3239 LP* 20 01 59.5133268456 +32 47 32.799122916   16.13 13.39 11.80 10.32 ~ 84 0
7 IRAS 20028+3910 pA* 20 04 35.9834860344 +39 18 44.208893700           F3-7I 65 0
8 V* QY Sge pA* 20 07 54.6224115384 +18 42 54.538913232   12.57       G0Ie 59 0
9 RAFGL 2699 C* 21 04 14.5277061504 +53 21 04.764238236     15.40     C8,3e 47 0

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