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Table 2
Line FWHM of the molecule of mean mass toward the Hi-GAL clumps (see Sect. 4.3.2).
| Clump type | Clump center | Ambient gas | |||
| [km s-1] | [km s-1] | ||||
|
|
|||||
| Starless | 1.3 ± 0.3 | 1.4 ± 0.5 | |||
| Protostellar | 1.8 ± 0.5 | 1.9 ± 0.3 | |||
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