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Table 1
Properties of the observed sources.
| Source | RA [J2000] | Dec [J2000] | vLSR | da | Mb | Lbolb | IR-8 μm | IR-22 μm |
| (km s-1) | (kpc) | (M⊙) | (L⊙) | |||||
|
|
||||||||
| G19.27+0.1M2 | 18:25:52.60 | –12:04:48.0 | 26.9 | 2.4 | 60 | 200 | quiet | quiet |
| G19.27+0.1M1 | 18:25:58.50 | –12:03:59.0 | 26.5 | 2.4 | 200 | 400 | quiet | quiet |
| G19.61–0.24A | 18:27:38.16 | –11:56:40.2 | 42.4 | 12.6c | 10 000d | 3 400 000d | loud | loud |
| G20.08–0.14 | 18:28:10:28 | –11:28:48.7 | 42.5 | 3.4e | 400a | 19 700a | loud | loud |
| IRAS 18264–1152 | 18:29:14.40 | –11:50:21.3 | 43.9 | 3.5 | 1600 | 19 000 | loud | loud |
| G23.60+0.0M1 | 18:34:11.60 | –08:19:06.0 | 106.5 | 6.2f | 1800 | 5200 | quiet | quiet |
| IRAS 18316–0602 | 18:34:20.46 | –05:59:30.4 | 42.5 | 3.1 | 1600 | 32 000 | loud | loud |
| G23.60+0.0M2 | 18:34:21.10 | –08:18:07.0 | 53.6 | 3.9 | 300 | 3000 | quiet | quiet |
| G24.33+0.1M1 | 18:35:07.90 | –07:35:04.0 | 113.6 | 6.7f | 2600 | 48 000 | quiet | loud |
| G25.04–0.2M1 | 18:38:10.20 | –07:02:34.0 | 63.8 | 4.3f | 400a | 1300a | quiet | quiet |
| G34.43+0.2M1 | 18:53:18.00 | +01:25:23.0 | 58.1 | 3.7 | 1400 | 24 000 | quiet | loud |
| IRAS 18507+0121 | 18:53:19.58 | +01:24:37.1 | 58.2 | 3.7 | 3100 | 14 500 | loud | loud |
| G34.43+0.2M3 | 18:53:20.40 | +01:28:23.0 | 59.4 | 3.7 | 600 | 1400 | quiet | quiet |
| IRAS 19095+0930 | 19:11:54.02 | +09:35:52.0 | 44.0 | 3.3 | 1000 | 50 600 | loud | loud |
| IRAS 18151–1208_2 | 18:17:50.50 | –12:07:55.0 | 29.8 | 3.0 | − | − | quiet | – |
Reference.
(d)
mass and bolometric luminosity from López-Sepulcre et al. (2011) for 3.8 kpc are rescaled to 12.6 kpc;
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