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Fig. 9

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Velocity integrated images of 12CO emission for clumps 2, 15, 16, 17, 18, 22, and 23, together with the corresponding dust continuum contours. The areas of all gas clumps are larger than the areas covered by dust. The red contours correspond to 3, 5, and 10σ, where σ is the rms of each velocity integrated image (Table 9). The white contours correspond to the 1.5 and 3σ contours of the ALMA 0.88 mm continuum image, as in Figure 6.

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