Table C.4
Visibility and density profiles in the ALMA sample.
| α1 | p1 | α2 | p2 | classification | |
|---|---|---|---|---|---|
| IRDC G11.11−4 1 | −0.42 ± 0.06 | 2.53 ± 0.06 | −0.06 ± 0.02 | 2.89 ± 0.02 | dust core |
| IRDC 18223−3 1 | −0.60 ± 0.05 | 2.26 ± 0.05 | −0.03 ± 0.01 | 2.83 ± 0.01 | dust core |
| IRDC 18223−3 2 | −0.61 ± 0.06 | 2.28 ± 0.06 | −0.01 ± 0.01 | 2.88 ± 0.01 | dust core |
| IRDC 18223−3 3 | −0.61 ± 0.06 | … | −0.02 ± 0.01 | … | dust core |
| IRDC 18223−3 4 | −0.61 ± 0.06 | … | −0.00 ± 0.01 | … | dust core |
| IRDC 18223−3 5 | −0.61 ± 0.06 | 2.22 ± 0.06 | −0.00 ± 0.01 | 2.83 ± 0.01 | dust core |
| IRDC 18223−3 6 | −0.61 ± 0.06 | 2.28 ± 0.06 | −0.00 ± 0.01 | 2.89 ± 0.01 | dust core |
| IRDC 18310−4 1 | −0.58 ± 0.07 | … | −0.00 ± 0.01 | … | dust core |
| HMPO IRAS 18089 1 | −0.49 ± 0.02 | 1.75 ± 0.10 | −0.49 ± 0.03 | 1.75 ± 0.10 | dust core |
| HMPO IRAS 18089 2 | −0.68 ± 0.02 | … | −0.11 ± 0.02 | … | dust core |
| HMPO IRAS 18089 3 | −0.66 ± 0.02 | 1.59 ± 0.14 | −0.12 ± 0.04 | 2.13 ± 0.15 | dust core |
| HMPO IRAS 18089 4 | −0.68 ± 0.02 | … | −0.07 ± 0.01 | … | dust core |
| HMPO IRAS 18182 1 | −0.42 ± 0.02 | 1.90 ± 0.07 | −0.43 ± 0.07 | 1.89 ± 0.10 | dust core |
| HMPO IRAS 18182 2 | −0.42 ± 0.01 | … | −0.46 ± 0.06 | … | dust core |
| HMPO IRAS 18182 3 | −0.45 ± 0.01 | 2.44 ± 0.04 | −0.39 ± 0.07 | 2.50 ± 0.08 | dust core |
| HMPO IRAS 18182 4 | −0.45 ± 0.02 | … | −0.39 ± 0.07 | … | dust core |
| HMPO IRAS 18264 1 | −0.72 ± 0.02 | 1.90 ± 0.04 | −0.19 ± 0.02 | 2.43 ± 0.04 | dust core |
| HMPO IRAS 18264 2 | −0.76 ± 0.03 | 2.02 ± 0.04 | −0.17 ± 0.02 | 2.61 ± 0.03 | dust core |
| HMPO IRAS 18264 3 | −0.85 ± 0.05 | 2.04 ± 0.05 | −0.13 ± 0.01 | 2.76 ± 0.02 | dust core |
| HMPO IRAS 18264 4 | −0.84 ± 0.05 | … | −0.14 ± 0.02 | … | dust core |
| HMPO IRAS 18264 5 | −0.82 ± 0.04 | 1.69 ± 0.06 | −0.09 ± 0.01 | 2.42 ± 0.04 | dust core |
| HMPOIRAS 18264 6 | −0.81 ± 0.04 | … | −0.10 ± 0.01 | … | dust core |
| HMPO IRAS 18264 7 | −0.81 ± 0.03 | … | −0.10 ± 0.02 | … | dust core |
| HMPO IRAS 18264 8 | −0.80 ± 0.04 | 1.80 ± 0.05 | −0.11 ± 0.02 | 2.49 ± 0.04 | dust core |
| HMPO IRAS 18264 9 | −0.83 ± 0.05 | … | −0.13 ± 0.02 | … | dust core |
| HMPO IRAS 18264 10 | −0.80 ± 0.04 | … | −0.11 ± 0.01 | … | dust core |
| HMPO IRAS 18264 11 | −0.80 ± 0.04 | 1.89 ± 0.04 | −0.10 ± 0.01 | 2.59 ± 0.02 | dust core |
| HMC G9.62+0.19 1 | −1.30 ± 0.12 | 1.03 ± 0.15 | −0.40 ± 0.04 | 1.93 ± 0.10 | dust±ff core |
| HMC G9.62+0.19 2 | −1.32 ± 0.10 | 0.95 ± 0.20 | −0.28 ± 0.03 | 1.99 ± 0.17 | dust±ff core |
| HMC G9.62+0.19 3 | −1.36 ± 0.07 | 1.04 ± 0.11 | −0.22 ± 0.06 | 2.18 ± 0.11 | dust core |
| HMC G9.62+0.19 4 | −1.30 ± 0.07 | … | −0.09 ± 0.05 | … | dust core |
| HMC G9.62+0.19 5 | −1.30 ± 0.07 | 1.00 ± 0.09 | −0.08 ± 0.05 | 2.22 ± 0.08 | dust core |
| HMC G9.62+0.19 6 | −1.26 ± 0.07 | … | −0.18 ± 0.05 | … | dust±ff core |
| HMC G9.62+0.19 7 | −1.27 ± 0.07 | 1.09 ± 0.09 | −0.09 ± 0.06 | 2.27 ± 0.08 | dust core |
| HMC G9.62+0.19 8 | −1.28 ± 0.07 | 1.38 ± 0.11 | −0.10 ± 0.05 | 2.56 ± 0.09 | dust core |
| HMC G9.62+0.19 9 | −1.29 ± 0.07 | … | −0.17 ± 0.04 | … | cometary UCHII region |
| HMC G9.62+0.19 10 | −1.29 ± 0.07 | … | −0.09 ± 0.05 | … | dust core |
| HMC G9.62+0.19 11 | −1.29 ± 0.07 | … | −0.09 ± 0.05 | … | dust core |
| HMC G10.47+0.03 1 | −0.19 ± 0.02 | 2.19 ± 0.13 | −0.64 ± 0.02 | 1.74 ± 0.13 | dust±ff core |
| HMC G10.47+0.03 2 | −0.23 ± 0.02 | 2.53 ± 0.06 | −0.61 ± 0.06 | 2.15 ± 0.08 | dust±ff core |
| HMC G10.47+0.03 3 | −0.23 ± 0.02 | 2.50 ± 0.19 | −0.56 ± 0.06 | 2.17 ± 0.20 | dust core |
| HMC G34.26+0.15 1 | −0.13 ± 0.03 | 2.19 ± 0.05 | −0.85 ± 0.06 | 1. 47 ± 0.07 | dust±ff core |
| HMC G34.26+0.15 2 | −0.18 ± 0.02 | 2.66 ± 0.04 | −0.52 ± 0.05 | 2.32 ± 0.06 | dust±ff core |
| HMC G34.26+0.15 3 | −0.18 ± 0.02 | … | −0.52 ± 0.06 | … | dust±ff core |
| HMC G34.26+0.15 4 | −0.17 ± 0.02 | 2.61 ± 0.04 | −0.53 ± 0.06 | 2.25 ± 0.07 | dust core |
| HMC G34.26+0.15 5 | −0.17 ± 0.02 | 2.59 ± 0.02 | −0.52 ± 0.06 | 2.24 ± 0.06 | dust core |
| UCHII G10.30-0.15 1 | −0.49 ± 0.06 | … | −1.06 ± 0.08 | … | cometary UCHII region |
| UCHII G13.87+0.28 1 | −1.80 ± 0.14 | 1.14 ± 0.14 | −0.32 ± 0.07 | 2.62 ± 0.08 | cometary UCHII region |
Notes. The visibility profiles are shown in Figs. 7 (HMC G9.62+0.19 2) and C.2 (all remaining sources). Two power-law profiles were fitted to the observed visibility profile with α1 and α2 tracing roughly the clump and core scales, respectively. The corresponding density power-law indices p1 and p1 (Eq. 2) are then estimated according to Eq. (5) considering the observed temperature power-law index q (Table C.2).
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