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Source | D |
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(pc) | (
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(km s-1) | (![]() |
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G10.47 | 1.25 | 0.57 | 1460-3200 | 5680 | 201 | 479001 | 0.57 | 44 |
G10.62 | 0.98 | 0.82 | 1920-4110 | 4770 | 201 | 202001 | 0.61 | 27 |
G16.59 | 0.77 | 0.69 | 390-870 | 1210 | 201 | 11301 | - | - |
G19.61 | 1.19 | 0.60 | 2450-5160 | 5320 | 201 | 330001 | - | - |
G23.44 | 1.79 | 0.76 | 2390-5120 | 2850 | 201 | 41601 | - | - |
G28.87 | 0.96 | 1.40 | 1260-2790 | 1350 | 332 | 34202 | - | - |
G29.96 | 1.34 | 0.56 | 2030-4460 | 2030 | 201 | 129001 | - | - |
G35.20 | 0.32 | 0.83 | 110-250 | 460 | 203 | 15003 | 0.66 | 14 |
G43.89 | 0.91 | 0.85 | 570-1200 | 2230 | 104 | 66104 | 0.86 | 88 |
G48.61 | 0.83 | 0.27 | 1200-2620 | 1280 | 295 | 37905 | - | - |
G75.78 | 0.54 | 0.41 | 450-1000 | 1390 | - | - | 0.68 | 23 |
a Optical depth of the C18O(2-1) emission, estimated from the 13CO(2-1) to C18O(2-1) line intensity ratio at the systemic velocity. b Clump mass estimated from the C18O(2-1) emission using the area under the whole emission line, and the spatial area delimited by the half power contour. ![]() c Virial mass, computed using Eq. (6) of Fontani et al. (2002). d Clump mass derived from the (sub)mm dust emission measured by the cited authors. e Rotational velocity; projected values (i.e. lower limits). f Dynamical mass of the clump, estimated using Eq. (3). References: 1 Hill et al. (2005), 2 Faúndez et al. (2004), 3 Mooney et al. (1995), 4 Hatchell et al. (2000), 5 Mueller et al. (2002). |
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