[tel-00726959, v1] Caractériser le milieu interstellaire ... - HAL - INRIA

E. Falgarone et al.: Extreme velocity-shears and CO on milliparsec scale 359tel-00726959, version 1 - 31 Aug 2012Fig. 3. From top to bottom, maps of the PdBI, PdBI+30m and 30m of 12 CO(1−0) emission integrated over the same velocity slices of 0.3 km s −1centered as indicated.up to ∼300 ′′ or 0.2 pc. In the case of structures #3, #4 and #5, theorientation of the edges of the large-scale patterns is more visiblein the 13 CO(1−0) maps (Fig. 9), likely because of the 12 CO(1−0)optical depth. This coincidence strongly suggests that the