Table 1
Sources observed.
| IRAS name | Other name | RA | Dec | d | b | V LSR | Ref. |
| J2000 | kpc | deg | km s-1 | ||||
|
|
|||||||
| 16552-3050 | GLMP 498 | 16:58:27.30 | −30:55:08.0 | 19.6 | + 7.3 | + 20 | 1, 2 |
| 18043-2116 | OH0.9-0.4 | 18:07:20.86 | −21:16:10.9 | 6.4 | −0.4 | + 90 | 3 |
| 18113-2503 | 18:14:27.27 | −25:03:00.5 | 6.7 or 10.0 | −3.6 | + 100 | 4 | |
| 18139-1816? | OH12.8-0.9 | 18:16:49.23 | −18:15:01.8 | – | −0.9 | + 60 | 5, 6 |
| 18286-0959 | 18:31:22.95 | −09:57:21.1 | 3.6 | −0.1 | + 41 | 7, 8 | |
| 18450-0148 | W43A | 18:47:41.16 | −01:45:11.5 | 2.6 | 0.0 | + 34 | 9,10 |
| 18460-0151 | OH31.0-0.2 | 18:48:43.02 | −01:48:30.5 | 2.1 | −0.2 | + 125 | 11, 12 |
| 18596+0315 | OH37.1-0.8 | 19:02:06.26 | +03:20:15.5 | 4.6 or 8.8 | −0.8 | + 90 | 13 |
| 19134+2131 | 19:15:35.22 | +21:36:33.9 | 8.0 | + 4.6 | − 65 | 14 | |
| 19190+1102 | 19:21:25.09 | +11:08:41.0 | 8.6 | −1.5 | + 20 | 15 | |
Notes. In bold face is given the most common name which is that used throughout this paper. Unclear association of IRAS 18139-1816 to OH12.8-0.9, probably due to wrong coordinates in the IRAS catalogue. Kinematic distances provided for IRAS 18113-2503 (see text). Unknown distance to OH12.8-0.9. Baud et al. (1985) proposed 8 kpc due to its membership to a group of evolved stars located towards the Galactic Centre.
Reference. (1) Suárez et al. (2007); (2) Suárez et al. (2008); (3) Deacon et al. (2007); (4) Gómez et al. (2011); (5) Engels et al. (1986); (6) Boboltz & Marvel (2005); (7) Imai et al. (2013a); (8) Yung et al. (2011); (9) Diamond et al. (1985); (10) Imai et al. (2005); (11) Deguchi et al. (2007); (12) Imai et al. (2013b); (13) Gómez et al. (1994); (14) Imai et al. (2007b); (15) Day et al. (2010).
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