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Fig. 2

image

Evolution of the radial profiles of the disks. Left: average gas surface density of the unperturbed disks after 12 Kyr (solid lines) compared to the initial distributions (thinner dashed lines) for various model setups, as indicated in the legend. The higher density and warmer models have constant kinematic viscosity ν (see text). Right: average gas temperature for the same models as in the left panel.

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