Table B.3
Calculated model parameter of NH3 (1,1) and NH3 (2,2) emission lines detected in 17 clumps.
Clump | Offset | Trot | Tkin | N(1, 1) | total-N(NH3) (a) | N(H2) (b) | χ(total-NH3) |
---|---|---|---|---|---|---|---|
(′, ′) | (K) | (K) | (cm−2) | (cm−2) | (cm−2) | ||
01 | (−17, −41) | 13.6 ± 2.9 | 14.9 ± 3.8 | 0.4 × 1014 | 3.8 × 1014 | 0.9 × 1022 | 4.3 × 10−8 |
02 | (1, −19) | 18.3 ± 2.4 | 22.5 ± 3.9 | 0.1 × 1014 | 0.3 × 1014 | 1.4 × 1022 | 0.2 × 10−8 |
03 | (9, 0) | 19.1 ± 2.1 | 23.2 ± 3.5 | 0.7 × 1014 | 3.6 × 1014 | 2.5 × 1022 | 1.4 × 10−8 |
04 | (30, −12) | 13.9 ± 1.6 | 15.5 ± 2.1 | 0.8 × 1014 | 6.5 × 1014 | 2.1 × 1022 | 3.1 × 10−8 |
05 | (22, −11) | 14.8 ± 1.2 | 16.8 ± 1.7 | 0.4 × 1013 | 0.3 × 1014 | 1.8 × 1022 | 0.2 × 10−8 |
06 | (17, −8) | 25.2 ± 4.3 | 34.9 ± 9.2 | 0.5 × 1013 | 0.2 × 1014 | 1.9 × 1022 | 0.1 × 10−8 |
07 | (1, 11) | 11.7 ± 0.6 | 12.5 ± 0.8 | 1.5 × 1014 | 1.9 × 1015 | 3.2 × 1022 | 5.9 × 10−8 |
08 | (0, 14) | 10.1 ± 1.2 | 10.6 ± 1.4 | 1.2 × 1014 | 2.3 × 1015 | 2.7 × 1022 | 8.9 × 10−8 |
09 | (4, 16) | 13.3 ± 0.6 | 14.6 ± 0.8 | 2.6 × 1014 | 2.3 × 1015 | 6.3 × 1022 | 3.7 × 10−8 |
10 | (6, 18) | 10.2 ± 0.7 | 10.7 ± 0.8 | 2.3 × 1014 | 4.3 × 1015 | 5.2 × 1022 | 8.3 × 10−8 |
11 | (9, 22) | 9.9 ± 0.6 | 10.5 ± 0.7 | 1.5 × 1014 | 2.9 × 1015 | 2.9 × 1022 | 9.9 × 10−8 |
12 | (12, 26) | 10.1 ± 0.4 | 10.6 ± 0.5 | 1.9 × 1014 | 3.8 × 1015 | 3.6 × 1022 | 1.1 × 10−7 |
13 | (13, 35) | 13.8 ± 0.9 | 15.2 ± 1.3 | 0.8 × 1014 | 6.4 × 1014 | 1.6 × 1022 | 4.1 × 10−8 |
14 | (21, 34) | 8.6 ± 1.6 | 8.9 ± 1.9 | 0.7 × 1014 | 2.5 × 1015 | 1.2 × 1022 | 2.1 × 10−7 |
15 | (23, 37) | 12.1 ± 1.9 | 13.0 ± 2.5 | 1.4 × 1014 | 1.6 × 1015 | 1.3 × 1022 | 1.2 × 10−7 |
16 | (19, 41) | 11.2 ± 0.4 | 11.9 ± 0.5 | 1.3 × 1014 | 1.8 × 1015 | 2.1 × 1022 | 8.5 × 10−8 |
17 | (25, 45) | 10.2 ± 0.7 | 10.7 ± 0.9 | 1.7 × 1014 | 3.2 × 1015 | 2.7 × 1022 | 1.2 × 10−7 |
Notes. (a) Total(para+ortho) column densities of NH3, see Sect. 3.4. (b) H2 column densities are taken from Bontemps et al. (2010) and Könyves et al. (2015). The central position is (l, b) = (28.59°, 3.55°). Offsets are based on Galactic coordinates.
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