Table 3
Parameters derived from the modified black-body fit of the SED down to 70 μm, and luminosity of the clumps (integrated from 1.2 mm and 3.6 μm).
| Clump | T d | 68% int. | M | 68% int. | β | 68% int. | L | 68% int. |
|
|
||||||||
| (K) | (K) | (102 × M⊙) | (102 × M⊙) | (102 × L⊙) | (102 × L⊙) | |||
|
|
||||||||
| 13560–6133c1 | 24.3 | 22.8−25.5 | 6.2 | 5.3−7.2 | 1.4 | 1.2−1.5 | 30.1 | 25.6−34.3 |
| 13563–6109c1 | 22.0 | 20.8−23.3 | 2.4 | 2.0−2.9 | 1.8 | 1.6−2.0 | 27.3 | 24.2−30.4 |
| 15072–5855c1 | 26.5 | 25.0−28.0 | 0.5 | 0.4−0.6 | 1.7 | 1.5−1.9 | 11.4 | 10.2−12.6 |
| 15278–5620c1 | 27.8 | 26.0−29.3 | 6.0 | 5.1−7.0 | 1.8 | 1.6−1.9 | 266.2 | 241.1−291.1 |
| 15278–5620c2 | 11.2 | 9.8−12.3 | 4.4 | 3.5−5.3 | 2.1 | 1.7−2.4 | 1.4 | 0.8−1.8 |
| 15470–5419c1 | 16.6 | 15.8−17.3 | 4.0 | 3.5−4.8 | 1.5 | 1.3−1.7 | 4.0 | 3.2−4.5 |
| 15470–5419c3 | 19.2 | 18.3−20.0 | 3.6 | 3.1−4.3 | 1.6 | 1.4−1.8 | 7.9 | 6.7−8.9 |
| 15557–5215c1 | 23.8 | 22.3−25.0 | 5.3 | 4.5−6.3 | 1.8 | 1.6−2.0 | 76.2 | 68.0−84.4 |
| 15557–5215c2 | 15.6 | 14.8−16.8 | 3.6 | 2.9−4.5 | 2.1 | 1.8−2.3 | 7.4 | 5.9−8.5 |
| 15579–5303c1 | 24.5 | 23.0−25.5 | 5.3 | 4.6−6.1 | 1.9 | 1.7−2.0 | 84.8 | 75.9−93.6 |
| 16061–5048c1 | 19.9 | 19.0−20.8 | 6.0 | 5.1−7.0 | 2.0 | 1.8−2.1 | 33.8 | 29.7−37.6 |
| 16061–5048c2 | 21.3 | 20.3−22.3 | 5.9 | 5.1−7.0 | 2.2 | 2.0−2.3 | 86.3 | 77.0−95.5 |
| 16061–5048c4 | 9.5 | 8.8−10.3 | 8.5 | 7.0−10.2 | 2.5 | 2.2−2.8 | 2.1 | 1.4−2.6 |
| 16093–5015c1 | 20.8 | 19.8−21.8 | 20.9 | 17.8−24.3 | 1.6 | 1.4−1.8 | 90.0 | 77.5−101.5 |
| 16093–5128c1 | 23.8 | 22.5−25.0 | 4.6 | 4.0−5.3 | 2.2 | 2.0−2.4 | 256.9 | 234.4−279.3 |
| 16093–5128c8 | 13.8 | 12.8−15.3 | 1.8 | 1.5−2.2 | 2.3 | 2.0−2.6 | 3.5 | 2.4−4.2 |
| 16254–4844c1 | 17.6 | 16.8−18.3 | 2.6 | 2.2−3.1 | 1.6 | 1.5−1.8 | 4.1 | 3.4−4.6 |
| 16573–4214c2 | 16.0 | 15.3−16.5 | 2.1 | 1.8−2.4 | 1.8 | 1.6−1.9 | 2.6 | 2.2−3.0 |
| 17040–3959c1 | 17.2 | 16.5−17.8 | 0.5 | 0.4−0.6 | 2.3 | 2.2−2.5 | 2.5 | 2.2−2.8 |
| 17355–3241c1 | 23.8 | 22.5−24.8 | 0.35 | 0.3−0.4 | 2.1 | 1.9−2.2 | 19.0 | 17.1−21.0 |
|
|
||||||||
| 14166–6118c2 | 18.1 | 15.3−20.8 | 0.5 | 0.4−0.6 | 1.7 | 1.2−2.0 | 1.3 | 0.8−1.7 |
| 14183–6050c3 | 16.1 | 15.0−17.0 | 1.0 | 0.7−1.2 | 1.9 | 1.6−2.3 | 2.3 | 1.5−2.7 |
| 15038–5828c1 | 12.2 | 11.3−13.3 | 5.4 | 4.5−6.5 | 2.1 | 1.8−2.4 | 3.3 | 1.9−3.8 |
| 15470–5419c4 | 11.1 | 10.3−12.0 | 6.2 | 5.1−7.5 | 2.4 | 2.0−2.6 | 2.9 | 1.9−3.7 |
| 15557–5215c3 | 9.6 | 8.5−10.5 | 3.6 | 2.9−4.5 | 2.9 | 2.5−3.3 | 1.8 | 1.1−2.6 |
| 15579–5303c3 | 15.6 | 14.5−17.0 | 3.4 | 2.7−4.3 | 1.6 | 1.3−1.9 | 3.9 | 2.1−4.8 |
| 16093–5128c2 | 10.4 | 9.0−11.5 | 5.1 | 4.0−6.1 | 2.7 | 2.3−3.0 | 3.2 | 1.7−4.0 |
| 16164–4929c3 | 9.2 | 8.3−10.3 | 4.7 | 3.8−5.7 | 2.6 | 2.2−2.9 | 1.0 | 0.6−1.7 |
| 16164–4929c6 | 11.0 | 10.3−12.0 | 1.1 | 0.9−1.4 | 2.4 | 2.1−2.7 | 0.7 | 0.4−1.0 |
| 16164–4837c2 | 8.1 | 7.5−8.8 | 3.2 | 2.7−3.9 | 3.0 | 2.7−3.4 | 0.8 | 0.5−1.0 |
| 16435–4515c3 | 10.5 | 9.8−11.3 | 4.3 | 3.5−5.1 | 2.7 | 2.4−2.9 | 2.9 | 1.8−3.6 |
| 16482–4443c2 | 8.7 | 8.0−9.5 | 1.9 | 1.6−2.3 | 3.1 | 2.8−3.5 | 0.8 | 0.5−1.0 |
Notes. The clumps above the horizontal line are those classified as star-forming, while the clump below it are those classified as quiescent (see Sect. 5). The columns shows the dust temperature (Td), the mass (M) of the gas and the dust emissivity index β from the modified black-body fit, and the luminosity of the clumps derived integrating the SED, with their uncertainties.
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