Table 4
Results of the fitting of the SEDs.
| Source | 70–500 μm | 850 μm (a) /870 μm (b) |  |
Tdust | θ | ||
|---|---|---|---|---|---|---|---|
| [1022 cm−2] | [K] | [″] | |||||
| 1 | I00117–MM1 | Y | – | (1.6 ± 0.7) × 1022 | 21 ± 4 | 27.8 | R |
| 2 | I00117–MM 2 | Y | – | (2.3 ± 1.0) × 1022 | 19 ± 3 | 23.9 | NR |
| 3 | AFGL5142–MM | Y | 850 | (1.2 ± 0.5) × 1023 | 26 ± 5 | 22.2 | R |
| 4 | AFGL5142–EC | Y | 850 | (8.0 ± 4.0) × 1022 | 27 ± 6 | 23.9 | NR |
| 5 | 05358–mm3 | – | – | – | – | ||
| 6 | 05358–mm1 | – | – | – | – | ||
| 7 | G5.89–0.39 | Y | 870 | (1.8 ± 0.8) × 1023 | 27 ± 5 | 40.8 | R |
| 8 | G008.14+0.22 | Y | 850 | (1.7 ± 0.6) × 1023 | 27 ± 4 | 30.0 | R |
| 9 | 18089−1732M1 | Y | 870 | (2.8 ± 1.0) × 1023 | 27 ± 4 | 17.5 | R |
| 10 | 18089−1732 M4 | Y | 850 | (4.8 ± 1.5) × 1022 | 22 ± 3 | 17.5 | R |
Notes.Availability of Herschel photometric data, SED fit results for the parameters
and
Tdust, angular dimension θ of the source from the 2D fitting at250 μm, and flag on the estimate of θ for the first ten sources of the sample. The SED fitting has been performed assuming β = 2. The full table is available via the CDS. (a)SCUBA Legacy Catalogues (Di Francesco et al. 2008); (b)ATLASGAL (Schuller et al. 2009; Csengeri et al. 2014); R = resolved sources; NR = unresolved sources for which we adopted θ =23.9′′.
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