Open Access

Fig. 5

image

Simulation of a full protoplanetary disk using given by Eq. (3) and running the code of Charnoz et al. (2019). Only the region around the snow-line is displayed. Solid lines in black, blue, and red represent the gas, water ice, and silicate dust surface densities (respectively), and the dashed blue line shows the water vapor. The black dots display the local sound velocity in m s−1 (right scale).

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