2006A&A...450.1051J


Query : 2006A&A...450.1051J

2006A&A...450.1051J - Astronomy and Astrophysics, volume 450, 1051-1059 (2006/5-2)

Near-infrared observations of water-ice in OH/IR stars.

JUSTTANONT K., OLOFSSON G., DIJKSTRA C. and MEYER A.W.

Abstract (from CDS):

A search for the near-infrared water-ice absorption band was made in a number of very red OH/IR stars which are known to exhibit the 10µm silicate absorption. As a by-product, accurate positions of these highly reddened objects are obtained. We derived a dust mass loss rate for each object by modelling the spectral energy distribution and the gas mass loss rate by solving the equation of motion for the dust drag wind. The derived mass loss rates show a strong correlation with the silicate optical depth as well as that of the water-ice. The stars have a high mass loss rate (>10–4M/yr) with an average gas-to-dust mass ratio of 110. In objects which show the 3.1 µm water-ice absorption, the near-IR slope is much steeper than those with no water-ice. Comparison between our calculated mass loss rates and those derived from OH and CO observations indicates that these stars have recently increased their mass loss rates.

Abstract Copyright:

Journal keyword(s): stars: AGB and post-AGB - stars: circumstellar matter - stars: evolution - stars: late-type - stars: mass-loss - infrared: stars

Simbad objects: 25

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Number of rows : 25
N Identifier Otype ICRS (J2000)
RA
ICRS (J2000)
DEC
Mag U Mag B Mag V Mag R Mag I Sp type #ref
1850 - 2024
#notes
1 OH 127.8-00.0 OH* 01 33 51.21048 +62 26 53.2032           O-rich 181 0
2 RAFGL 5379 OH* 17 44 24.0074369832 -31 55 35.414175828           O-rich 88 0
3 PN Sa 3-96 PN 17 55 45.05304 -15 03 42.8220           O-rich 44 2
4 OH 010.04-00.10 OH* 18 08 16.38432 -20 16 11.5608           O-rich 33 0
5 IRAS 18092-2347 OH* 18 12 20.42280 -23 46 55.7796           O-rich 17 0
6 IRAS 18100-1915 OH* 18 13 03.08064 -19 14 18.8700           O-rich 25 0
7 OH 016.1-00.3 OH* 18 21 06.97512 -15 03 21.6864           O-rich 48 0
8 OH 020.7+00.1 OH* 18 28 30.83160 -10 50 52.5912           O-rich 49 0
9 OH 021.5+00.5 OH* 18 28 30.93720 -09 58 14.3184           O-rich 93 0
10 IRAS 18310-2834 OH* 18 34 13.77576 -28 32 21.5988           O-rich 14 0
11 OH 024.7+00.3 OH* 18 35 29.21616 -07 13 10.9740           O-rich 38 0
12 OH 026.5+00.6 OH* 18 37 32.50920 -05 23 59.1936           O-rich 301 1
13 OH 025.5-00.3 OH* 18 38 50.54280 -06 44 49.6068           O-rich 24 0
14 IRAS 18361-0647 mul 18 38 50.7 -06 44 54           ~ 22 0
15 OH 030.7+00.4 OH* 18 45 52.39728 -01 46 42.4776           O-rich 69 1
16 OH 030.1-00.7 OH* 18 48 41.98728 -02 50 29.5080           O-rich 100 0
17 OH 032.0-00.5 OH* 18 51 26.25600 -01 03 52.3620           O-rich 68 0
18 OH 032.8-00.3 OH* 18 52 22.25472 -00 14 11.8428           O-rich 123 0
19 IRAS 18588+0428 OH* 19 01 20.05464 +04 32 31.5780           O-rich 17 0
20 OH 039.9-00.0 OH* 19 04 09.74928 +06 13 16.3956           O-rich 64 0
21 OH 042.3-00.1 OH* 19 09 08.32632 +08 16 33.6504           O-rich 87 0
22 OH 051.8-00.2 OH* 19 27 42.03672 +16 37 23.9520           O-rich 40 0
23 OH 065.7-00.8 OH* 19 59 39.14304 +28 23 07.2996           O-rich 33 0
24 OH 075.3-01.8 OH* 20 29 08.58696 +35 45 43.4916           O-rich 40 0
25 RAFGL 2885 OH* 22 19 27.47784 +59 51 21.7080           O-rich 136 0

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