Table 4
Summary of the properties derived from the fit of the Robitaille models to the SED of the objects with significant mid-IR emission.
| Clump | M ∗ | L Rob | L | M env |
| (M⊙) | (102 × L⊙) | (102 × L⊙) | (102 × M⊙) | |
|
|
||||
| 13560–6133c1 | 9.6−15.4 | 25−43 | 26−34 | 15.0−36.0 |
| 13563–6109c1 | 9.7−13.8 | 27−49 | 24−30 | 5.5−18.0 |
| 15072–5855c1 | 5.9−8.8 | 6−28 | 10−13 | 1.6−15.0 |
| 15278–5620c1 | 14.7−22.9 | 307−665 | 241−291 | 16.0−28.0 |
| 15557–5215c1 | 10.1−27.4 | 37−234 | 68−84 | 5.2−23.0 |
| 15557–5215c2 | 6.0−9.6 | 6−15 | 6−9 | 7.3−15.0 |
| 15579–5303c1 | 13.4−17.8 | 149−334 | 76−94 | 14.0−34.0 |
| 16061–5048c1 | 12.5−18.5 | 52−116 | 30−38 | 23.0−40.0 |
| 16061–5048c2 | 11.0−24.4 | 83−781 | 77−96 | 16.0−21.0 |
| 16093–5015c1 | 12.8−21.9 | 45−209 | 78−102 | 19.0−52.0 |
| 16093–5128c1 | 14.8−24.2 | 104−638 | 234−279 | 9.8−40.0 |
| 17195–3811c1 | 9.3−12.9 | 23−138 | − | 7.2−31.0 |
| 17355–3241c1 | 7.6−8.2 | 21−34 | 17−21 | 2.2−2.5 |
Notes. Our estimated range in L is shown for comparison. The ranges in M∗, LRob and Menv are those spanned by the best ten models. The masses are derived with a different dust model, and thus deviate from our estimate.
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