Fig. 12
Time scales depending on the distance from the central star for 0.005 M⊙, 0.010 M⊙, 0.015 M⊙ and 0.040 M⊙ discs. To compute the time scales we used the density and temperature of the midplane at the beginning of the fully radiative simulations (when the disc is in the r − θ equilibrium between viscous heating and radiative transport/cooling).
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