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Fig. 11

image

Circularly averaged radial column density profiles centred on the studied clumps. The column density is plotted as a function of pixel (each pixel is an azimuthal average) distance from the centre. The error bars display the standard deviation onthe azimuthal average at each pixel. Saturated proto-stellar clumps are plotted separately because the fluxes are modelled and recovered from Gaussian fitting.

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