Fig. 5
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Each data point represents the ratio, R = F(2O)∕F(O), at the spatial resolutions O and 2O of either the number (top, F = NB) or mean mass (bottom, 
) of sources, and plotted at the mean spatial resolution x = 3O∕2. The left panels correspond to the observations of Aquila and NGC 6334. The right panels correspond to the numerical models.
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