Table E.1.
Characteristic parameters of the DCN (3-2) hyperfine fits for the non-background subtracted.
| Protocluster | Number1 | Number2 | Detection2 | Velocity3 | VLSR3 | VLSR3 | Linewidth3 | Linewidth3 | Linewidth3 |
|---|---|---|---|---|---|---|---|---|---|
| cloud name | of Cores | detected | rate [%] | range | mean | std | mean | median | std |
| (complex) | (complex) | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | [km s−1] | ||
| Young | |||||||||
| G327.29 | 32 | 18 (23) | 56 (72)% | 5.3 | -44.9 | 1.9 | 1.7 | 1.7 | 0.5 |
| G328.25 | 11 | 3 (4) | 27 (36)% | 1.4 | -43.1 | 0.6 | 1.9 | 1.6 | 0.9 |
| G338.93 | 42 | 21 (29) | 50 (69)% | 6.9 | -60.9 | 2.0 | 2.1 | 2.0 | 0.7 |
| G337.92 | 22 | 10 (17) | 45 (77)% | 4.0 | -39.2 | 1.3 | 2.1 | 2.0 | 1.1 |
| W43-MM1 | 70 | 32 (51) | 46 (73)% | 7.5 | 97.2 | 2.1 | 1.9 | 1.6 | 1.1 |
| W43-MM2 | 40 | 23 (30) | 58 (75)% | 4.3 | 90.8 | 1.3 | 1.9 | 1.6 | 0.9 |
| Average | 36 | 18(26) | 49 (71)% | 4.9 | 1.8 | 1.9 | 1.7 | 0.9 | |
| Total | 217 | 107 (154) | |||||||
| Intermediate | |||||||||
| G351.77 | 18 | 5 (14) | 28 (78)% | 5.9 | -4.5 | 2.1 | 2.0 | 1.6 | 0.6 |
| G353.41 | 45 | 17 (22) | 38 (49)% | 7.4 | -17.3 | 1.8 | 1.7 | 1.5 | 0.8 |
| G008.67 | 19 | 8 (13) | 42 (68)% | 6.6 | 35.8 | 2.0 | 2.0 | 1.9 | 0.6 |
| W43-MM3 | 36 | 12 (18) | 33 (50)% | 2.6 | 93.1 | 0.8 | 1.8 | 2.0 | 0.7 |
| W51-E | 23 | 12 (21) | 52 (91)% | 11.1 | 56.8 | 3.9 | 2.0 | 1.6 | 1.0 |
| Average | 28 | 11(18) | 38 (62)% | 6.7 | 2.8 | 1.8 | 1.6 | 0.8 | |
| Total | 141 | 54 (88) | |||||||
| Evolved | |||||||||
| G333.60 | 52 | 36 (42) | 69 (81)% | 10.0 | -47.8 | 1.9 | 1.7 | 1.7 | 0.5 |
| G010.62 | 42 | 28 (37) | 67 (88)% | 9.3 | -2.5 | 2.1 | 1.4 | 1.3 | 0.6 |
| G012.80 | 46 | 38 (40) | 83 (87)% | 6.4 | 36.1 | 1.4 | 1.4 | 1.2 | 0.6 |
| W51-IRS2 | 97 | 69 (84) | 71 (87)% | 18.3 | 61.9 | 2.9 | 1.5 | 1.3 | 0.8 |
| Average | 59 | 43 (51) | 72 (86)% | 11.0 | 2.5 | 1.5 | 1.3 | 0.7 | |
| Total | 237 | 171 (203) | |||||||
The number of continuum cores is taken from the smoothed core catalogue from Louvet et al. (2023).
The number of cores detected and the detection rates (given in percentages) are for single-type DCN detections. The numbers within the brackets are for the sum of the single- and complex-type DCN detections. Spectra described as complex-type spectra are not well fit by a single component. We provide the percentages and number of detections, but cores with a complex-type spectrum are not included in the estimates of the velocity range, VLSR, or linewidth.
Only single-type DCN spectra (fit with a single component) and listed as single in the Tables of the DCN fits (e.g. Table 3) are included in the estimates of the velocity ranges, VLSR and linewidth for each protocluster.
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