Table 1
Types of [C I] 492 GHz and 13CO(21) detections.
| Type 0(a) | Type 1(a) | Type 2(a) | |
|---|---|---|---|
| [C I] detection | ✓ | ✕ | ✓ |
| 13CO detection | ✓ | ✓ | ✕ |
| 70w | 14 (10) | 0 | 0 |
| IRw | 31 (21) | 0 | 0 |
| IRb | 31 (21) | 0 | 0 |
| H II region | 22 (22) | 0 | 0 |
| Diffuse(b) | 35 (23) | 45 (42) | 5 (3) |
| Total | 133 (97) | 45 (42) | 5 (3) |
Notes. (a)The values in parenthesis are the numbers of detections that have clean reference positions. (b)G22.37+0.45 shows two components in [C I] 492 GHz, which are sufficiently close to be considered as one component in 13CO(21). When we compared [C I] 492 GHz to13 CO(21), we therefore used a sum of the two components in [C I] 492 GHz for this source. Because of this, the total number of diffuse cloud components detected in [C I] 492 GHz is 40 in this table, as opposed to 41 as we mentioned in Sect. 3.4.
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