Table 7
Modelling parameters.
| # | Source | n0 | p | ⟨n⟩ | α | T0 | ⟨T⟩ |
| (grains m-3) | (cm-3) | (K) | (K) | ||||
|
|
|||||||
| 1 | IRAS 05358+3543 | 1.5 × 103 | 1.4 | 8.4 × 105 | −0.62 | 562 | 31.1 |
| 2 | IRAS 18089−1732 | 7.4 × 104 | 1.5 | 6.1 × 107 | −0.46 | 407 | 36.1 |
| 3 | IRAS 18151−1208-MM1 | 8.7 × 102 | 1.2 | 5.5 × 105 | −0.60 | 631 | 32.5 |
| 4 | IRAS 18151−1208-MM2 | 7.5 × 102 | 1.3 | 6.5 × 105 | −0.61 | 427 | 24.2 |
| 5 | IRAS 18264−1152 | 4.0 × 103 | 1.5 | 9.8 × 105 | −0.61 | 676 | 32.6 |
| 6 | W43-MM1 | 2.0 × 105 | 2.0 | 5.5 × 106 | −0.54 | 302 | 20.0 |
| 7 | DR21(OH) | 4.1 × 104 | 1.5 | 3.5 × 107 | −0.44 | 191 | 20.7 |
| 8 | DR21(OH)-S | 1.8 × 104 | 1.5 | 1.5 × 107 | −0.43 | 224 | 25.3 |
| 9 | NGC 7538S | 2.9 × 104 | 1.5 | 2.4 × 107 | −0.45 | 316 | 30.4 |
| 10 | IRAS 23385+6053 | 5.4 × 105 | 1.5 | 5.0 × 108 | −0.42 | 347 | 38.7 |
Notes. Table presents the source name, the number of dust grains n0 per meter cube at r0 = 100 AU (following a standard MRN distribution in size and types), the power-law index p, the mean H2 density in the source, the best-fit temperature distribution coefficients (T = T0(r/r0)α) and the mean temperature in the source.
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