Table C.1
Properties of each clump, averaged within the FWHM 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 | 1.1 | 0.7−1.2 | 26.0 | 17.8−30.5 | 9.0 | 6.1−10.5 | 2.29 | 1.57−2.69 | 0.3 | |
| 12300−6119c1 | 1.4 | 1.1−1.7 | 10.5 | 7.9−12.4 | 5.4 | 4.1−6.4 | 1.39 | 1.04−1.64 | 0.5 | |
| 13560−6133c1 | 4.5 | 2.5−5.7 | 41.5 | 22.7−52.5 | 19.9 | 10.9−25.1 | 5.09 | 2.79−6.43 | 0.5 | |
| 15072−5855c1 | 0.6 | 0.3−0.8 | 10.8 | 5.5−13.5 | 4.2 | 2.1−5.3 | 1.07 | 0.54−1.35 | 0.4 | |
| 15278−5620c1 | 5.9 | 4.7−6.9 | 187.0 | 150.0−220.0 | 59.0 | 47.4−69.7 | 15.10 | 12.10−17.80 | 0.3 | |
| 15278−5620c2 | 1.7 | 1.3−2.0 | 5.1 | 4.0−6.1 | 3.5 | 2.8−4.2 | 0.90 | 0.71−1.08 | 0.7 | |
| 15470−5419c1 | 2.5 | 1.2−3.1 | 22.4 | 10.3−27.3 | 10.8 | 5.0−13.2 | 2.77 | 1.27−3.38 | 0.5 | |
| 15470−5419c3 | 5.0 | 4.1−5.8 | 4.0 | 3.3−4.6 | 4.3 | 3.6−5.0 | 1.11 | 0.91−1.28 | 1.1 | |
| 15557−5215c1 | 7.3 | 3.1−9.0 | 20.9 | 8.7−25.5 | 14.8 | 6.1−18.0 | 3.78 | 1.57−4.62 | 0.7 | |
| 15557−5215c2 | 3.7 | 2.9−4.4 | 13.0 | 10.1−15.5 | 8.5 | 6.7−10.2 | 2.19 | 1.70−2.61 | 0.7 | |
| 15579−5303c1 | 2.7 | 2.3−3.2 | 38.0 | 31.7−43.8 | 15.8 | 13.2−18.3 | 4.06 | 3.39−4.68 | 0.4 | |
| 16061−5048c1 | 2.1 | 1.6−2.6 | 36.5 | 26.7−44.5 | 14.2 | 10.4−17.3 | 3.63 | 2.66−4.43 | 0.4 | |
| 16061−5048c2 | 2.9 | 2.4−3.3 | 22.3 | 18.5−26.1 | 11.3 | 9.3−13.2 | 2.89 | 2.39−3.37 | 0.5 | |
| 16061−5048c4 | 3.6 | 2.9−4.3 | 5.6 | 4.6−6.6 | 4.9 | 4.0−5.8 | 1.25 | 1.01−1.47 | 0.9 | |
| 16093−5015c1 | 22.1 | 17.0−25.5 | 2.9 | 2.2−3.3 | 5.7 | 4.4−6.6 | 1.46 | 1.13−1.69 | 2.0 | |
| 16093−5128c1 | 5.6 | 4.5−6.6 | 13.5 | 10.8−15.9 | 10.1 | 8.0−11.8 | 2.58 | 2.06−3.03 | 0.8 | |
| 16093−5128c8 | 8.5 | 2.2−10.0 | 1.9 | 0.5−2.2 | 3.1 | 0.8−3.7 | 0.81 | 0.21−0.95 | 1.7 | |
| 16254−4844c1 | 1.3 | 0.9−1.7 | 43.2 | 30.9−55.8 | 13.6 | 9.7−17.5 | 3.47 | 2.49−4.49 | 0.3 | (1) |
| 16428−4109c1 | 1.9 | 1.5−2.2 | 13.8 | 10.9−15.6 | 7.2 | 5.6−8.1 | 1.83 | 1.44−2.07 | 0.5 | |
| 16428−4109c2 | 1.5 | 1.3−1.7 | 8.3 | 7.1−9.5 | 4.7 | 4.0−5.4 | 1.21 | 1.03−1.38 | 0.6 | |
| 16573−4214c2 | 1.1 | 0.8−1.3 | 174.0 | 128.0−208.0 | 32.2 | 23.6−38.4 | 8.25 | 6.04−9.84 | 0.2 | (1) |
| 17040−3959c1 | 0.4 | 0.3−0.5 | 47.5 | 38.0−56.0 | 9.7 | 7.7−11.4 | 2.47 | 1.98−2.91 | 0.2 | (2) |
| 17195−3811c1 | 2.3 | 1.1−2.7 | 10.9 | 5.1−13.2 | 6.5 | 3.0−7.8 | 1.65 | 0.78−2.00 | 0.6 | |
| 17195−3811c2 | 2.9 | 2.4−3.3 | 14.0 | 11.7−15.7 | 8.3 | 6.9−9.3 | 2.13 | 1.78−2.38 | 0.6 | |
| 17195−3811c3 | 3.7 | 3.0−4.2 | 5.0 | 4.0−5.7 | 4.5 | 3.7−5.2 | 1.15 | 0.94−1.33 | 0.9 | |
| 17355−3241c1 | 0.15 | 0.1−0.2 | 3.3 | 2.5−3.9 | 1.2 | 0.9−1.5 | 0.31 | 0.24−0.37 | 0.4 | |
|
|
||||||||||
| 13560−6133c2 | 4.5 | 1.4−5.5 | 20.1 | 6.4−24.8 | 12.2 | 3.9−15.1 | 3.13 | 1.00−3.86 | 0.6 | |
| 14166−6118c2 | 1.1 | 0.7−1.3 | 7.6 | 5.3−9.1 | 4.0 | 2.8−4.8 | 1.01 | 0.71−1.22 | 0.5 | |
| 14183−6050c3 | 4.2 | 1.8−4.7 | 5.2 | 2.2−5.9 | 4.9 | 2.1−5.5 | 1.25 | 0.53−1.40 | 1.0 | |
| 15038−5828c1 | 1.6 | 1.2−1.9 | 24.9 | 18.7−29.8 | 10.0 | 7.5−12.0 | 2.56 | 1.92−3.07 | 0.4 | |
| 15470−5419c4 | 4.8 | 2.6−6.1 | 4.3 | 2.4−5.4 | 4.5 | 2.5−5.7 | 1.14 | 0.63−1.45 | 1.1 | |
| 15557−5215c3 | 2.1 | 1.6−2.5 | 1.6 | 1.2−2.0 | 1.8 | 1.4−2.1 | 0.45 | 0.34−0.55 | 1.1 | |
| 15579−5303c3 | 5.1 | 2.9−6.3 | 10.2 | 5.8−12.7 | 8.1 | 4.6−10.1 | 2.08 | 1.18−2.57 | 1.1 | |
| 16093−5128c2 | 3.6 | 2.4−4.4 | 6.6 | 4.5−8.1 | 5.4 | 3.7−6.6 | 1.37 | 0.93−1.69 | 0.8 | |
| 16164−4929c3 | 3.2 | 2.1−4.0 | 7.3 | 4.7−9.1 | 5.6 | 3.6−6.9 | 1.43 | 0.92−1.78 | 0.8 | |
| 16482−4443c2 | 0.4 | 0.2−0.5 | 47.4 | 19.6−57.0 | 10.0 | 4.1−12.0 | 2.56 | 1.06−3.08 | <0.2 | (3) |
Notes. The columns show respectively: clump name, mass, volume- and column-density of H2, mass surface density, with their 68% credibility interval, and the beam-corrected 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. (3) Volume-, column- and surface-densities are lower limits, as the source is unresolved.
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