Table 1
Cloud complexes and their properties.
| Complex | Dfga | Dgenb | Dgrsc | MNIR [104M⊙] | MCO/MNIRd | M8 μm/MNIR [%] | M870 μm/MNIR [%] |
|
|
|||||||
| 03.80 − 01.00 | 2.5 | – | – | 1.7 | – | – | 12 |
| 11.10 − 00.10 | 4.1 | 4.74 | 3.6 | 4.5 | – | 11 | 15 |
| 18.54 − 00.16 | 5.9 | 4.33 | 4.1 | 4.7 | 1.1 | 17 | 22 |
| 24.94 − 00.16 | 3.5 | – | 3.41 | 3.6 | 2.7 | 10 | 10 |
| 32.09 + 00.09 | 8.0 | 7.45 | 7.1 | 12 | 1.5 | 29 | 26 |
| 34.24 + 00.14 | 5.9 | – | 3.8 | 13 | 2.7 | 46 | 51 |
| 34.39 − 00.71 | 0.7 | – | 1 | 0.9 | 0.3 | 0 | 3 |
| 35.49 − 00.31 | 3.2 | 3.63 | 3.0 | 5.6 | 0.7 | 8 | 7 |
| 36.74 − 00.16 | 5.1 | 3.88 | 3.6 | 5.4 | 1.7 | 7 | 14 |
| 38.94 − 00.46 | 2.7 | 4.14 | 10.5 | 2.0 | 1.6 | 50 | 14 |
Notes.
Distance derived from the foreground source densities in this paper (see Sect. 3).
Distance derived from modeling of NIR source color distribution by Marshall et al. (2009).
Unless otherwise stated, the distance is a kinematic distance from the GRS survey (Roman-Duval et al. 2009).
As estimated in Roman-Duval et al. (2010), corrected to correspond to the distance Dfg listed in Col. 2.
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