Table C.2
Properties of each clump, averaged within the 3σ contour.
| Clump | M | 68% int. | n(H2) | 68% int. | N(H2) | 68% int. | Σ | 68% int. | Diameter | Notes |
|
|
||||||||||
| (102 × M⊙) | (104 × cm-3) | (1022 × cm-2) | (10-1 × g cm-2) | (pc) | ||||||
|
|
||||||||||
| 08477−4359c1 | 2.3 | 1.7−2.6 | 4.1 | 3.1−4.6 | 3.4 | 2.5−3.8 | 0.87 | 0.65−0.98 | 0.8 | |
| 12300−6119c1 | 2.7 | 2.0−3.2 | 1.8 | 1.4−2.1 | 2.1 | 1.6−2.5 | 0.53 | 0.40−0.63 | 1.2 | |
| 13560−6133c1 | 12.0 | 8.2−16.0 | 1.7 | 1.1−2.1 | 3.3 | 2.2−4.2 | 0.85 | 0.56−1.10 | 2.0 | |
| 15072−5855c1 | 1.4 | 0.8−1.8 | 2.0 | 1.0−2.5 | 1.8 | 0.9−2.3 | 0.46 | 0.24−0.58 | 0.9 | |
| 15278−5620c1 | 14.0 | 12.0−17.0 | 2.8 | 2.3−3.3 | 4.9 | 4.0−5.6 | 1.20 | 1.00−1.40 | 1.8 | |
| 15278−5620c2 | 3.0 | 2.6−3.3 | 1.6 | 1.4−1.8 | 2.0 | 1.8−2.2 | 0.51 | 0.45−0.57 | 1.3 | |
| 15470−5419c1 | 5.0 | 2.5−6.0 | 3.0 | 1.5−3.6 | 3.6 | 1.8−4.3 | 0.91 | 0.45−1.10 | 1.2 | |
| 15470−5419c3 | 11.0 | 10.0−11.0 | 1.0 | 1.0−1.1 | 2.2 | 2.2−2.4 | 0.57 | 0.55−0.61 | 2.2 | |
| 15557−5215c1 | 21.0 | 10.0−26.0 | 2.4 | 1.2−2.9 | 4.9 | 2.5−6.1 | 1.30 | 0.63−1.60 | 2.1 | |
| 15557−5215c2 | 8.4 | 7.5−9.5 | 1.4 | 1.2−1.6 | 2.5 | 2.3−2.9 | 0.65 | 0.58−0.73 | 1.9 | |
| 15579−5303c1 | 8.1 | 7.8−8.7 | 1.2 | 1.2−1.3 | 2.3 | 2.2−2.5 | 0.60 | 0.57−0.63 | 1.9 | |
| 16061−5048c1 | 5.2 | 4.3−6.2 | 1.7 | 1.4−2.0 | 2.5 | 2.1−3.0 | 0.64 | 0.53−0.76 | 1.5 | |
| 16061−5048c2 | 5.7 | 4.9−6.7 | 2.8 | 2.4−3.3 | 3.6 | 3.1−4.2 | 0.92 | 0.79−1.10 | 1.3 | |
| 16061−5048c4 | 6.3 | 5.7−6.7 | 1.9 | 1.7−2.0 | 2.8 | 2.5−3.0 | 0.71 | 0.65−0.77 | 1.5 | |
| 16093−5015c1 | 54.2 | 48.2−59.1 | 0.4 | 0.3−0.5 | 2.0 | 1.8−2.2 | 0.51 | 0.45−0.56 | 5.3 | |
| 16093−5128c1 | 12.0 | 11.0−14.0 | 2.1 | 1.9−2.3 | 3.8 | 3.4−4.2 | 0.97 | 0.86−1.10 | 1.9 | |
| 16093−5128c8 | 10.0 | 3.4−12.0 | 1.2 | 0.4−1.4 | 2.5 | 0.8−3.0 | 0.65 | 0.21−0.76 | 2.1 | |
| 16254−4844c1 | 2.3 | 1.9−3.0 | 2.3 | 1.9−3.0 | 2.3 | 1.9−3.0 | 0.60 | 0.48−0.77 | 1.0 | (1) |
| 16428−4109c1 | 8.1 | 6.6−9.3 | 1.1 | 0.9−1.2 | 2.1 | 1.7−2.4 | 0.53 | 0.43−0.62 | 2.0 | |
| 16428−4109c2 | 4.8 | 4.2−5.6 | 0.8 | 0.7−1.0 | 1.5 | 1.3−1.8 | 0.39 | 0.34−0.45 | 1.8 | |
| 16573−4214c2 | 1.7 | 1.4−2.0 | 8.8 | 7.2−10.0 | 5.1 | 4.2−6.0 | 1.30 | 1.10−1.50 | 0.6 | (1) |
| 17040−3959c1 | 0.6 | 0.6−0.7 | 6.3 | 5.7−6.9 | 3.0 | 2.6−3.2 | 0.75 | 0.68−0.83 | 0.5 | (2) |
| 17195−3811c1 | 6.5 | 3.6−7.8 | 1.6 | 0.9−1.9 | 2.6 | 1.4−3.1 | 0.66 | 0.36−0.80 | 1.6 | |
| 17195−3811c2 | 8.3 | 8.0−8.5 | 2.1 | 2.0−2.1 | 3.3 | 3.2−3.4 | 0.85 | 0.81−0.86 | 1.6 | |
| 17195−3811c3 | 6.3 | 5.5−6.8 | 1.8 | 1.6−2.0 | 2.8 | 2.4−3.0 | 0.71 | 0.63−0.77 | 1.5 | |
| 17355−3241c1 | 0.3 | 0.2−0.3 | 1.7 | 1.4−1.9 | 0.9 | 0.8−1.0 | 0.24 | 0.20−0.27 | 0.6 | |
|
|
||||||||||
| 13560−6133c2 | 8.1 | 2.9−9.1 | 3.5 | 1.2−3.9 | 4.6 | 1.7−5.2 | 1.20 | 0.43−1.30 | 1.4 | |
| 14166−6118c2 | 1.4 | 1.1−1.6 | 5.1 | 3.9−6.0 | 3.3 | 2.5−3.9 | 0.85 | 0.65−0.99 | 0.7 | |
| 14183−6050c3 | 5.4 | 2.3−5.9 | 3.2 | 1.4−3.6 | 3.9 | 1.6−4.2 | 0.99 | 0.41−1.10 | 1.2 | |
| 15038−5828c1 | 4.6 | 3.8−5.3 | 2.2 | 1.9−2.5 | 2.9 | 2.4−3.2 | 0.73 | 0.61−0.83 | 1.3 | |
| 15470−5419c4 | 6.2 | 3.7−7.7 | 2.6 | 1.6−3.2 | 3.5 | 2.1−4.3 | 0.89 | 0.53−1.10 | 1.4 | |
| 15557−5215c3 | 2.0 | 1.7−2.4 | 1.6 | 1.3−1.8 | 1.7 | 1.4−2.0 | 0.44 | 0.37−0.51 | 1.1 | |
| 15579−5303c3 | 10.0 | 6.1−12.0 | 1.4 | 0.9−1.7 | 2.8 | 1.7−3.3 | 0.71 | 0.42−0.86 | 2.0 | |
| 16093−5128c2 | 5.1 | 3.7−5.9 | 2.7 | 2.0−3.1 | 3.3 | 2.5−3.9 | 0.86 | 0.63−0.99 | 1.3 | |
| 16164−4929c3 | 5.4 | 3.4−6.8 | 2.5 | 1.6−3.2 | 3.3 | 2.0−4.1 | 0.84 | 0.52−1.05 | 1.3 | |
| 16482−4443c2 | 0.8 | 0.3−1.0 | 7.8 | 3.1−9.3 | 3.7 | 1.5−4.4 | 0.94 | 0.38−1.10 | 0.5 | |
Notes. The columns show respectively: clump name, mass, volume- and column-density of H2, mass surface density, with their 68% credibility interval, and the diameters of the clumps. The clumps above the horizontal line are those classified as star-forming, while the clumps below it are those classified as quiescent. (1) Source with very poor uv-coverage in NH3: spectrum extracted from non-cleaned maps. (2) Lower limit for the mass and the derived quantities.
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