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Fig. 4


Left panels. Histograms showing the distribution of ln(M) for all (black), starless (red) and proto-stellar (blue) clumps in the  = 30° (top) and  = 59° (bottom) fields. The solid lines represent the results of Gaussian fits to the histograms. The vertical solid lines represent the completeness limits as in Fig. 3. Vertical bars show Poisson errors. Right panels. PDFs of the mass distribution (black solid line) and best-fit (red dashed line), in the  = 30° (top) and  = 59° (bottom) fields.

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