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Fig. 14

image

Comparison between our fiducial model (shaded regions) and two other models with different optical depths: an optically thin case (TS = 8000 K, dot-dashed lines) and a more optically thick one (TS = 80 K, dashed lines). From top to bottom: rotation velocity, velocity dispersion, midplane density, scale height and surface density as a function of R. Only the averaged profiles are shown, smoothed at the spatial resolution of 0.2 kpc. Different regimes predict significantly different column densities.

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