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Fig. 1

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DGMFs of four simulations (black lines) with ℳs = 10, processed to mimic those observed with a near-infrared dust extinction mapping technique. The solid lines show the DGMFs at t = 0 and the dotted lines at time steps SFE =  { 1,3,10 } %. The panels also show with dashed lines the mean DGMF of nearby starless clouds (blue) and of Taurus (Kainulainen et al. 2009, red), and of a sample of IRDCs (KT13, green).

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