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Fig. D.1.

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Radial profiles for the model with start = 1.0 × 10−8 M yr−1 at the starting point of the simulation, t0 = 2 Myr (left column), as well as at 5.0 Myr (center column) and 8.0 Myr (right column). The solid (dashed) lines correspond to a metallicity of Z = 1 Z (Z = 0.2 Z). Panel (a) shows the disk surface density, Σ, panel (b) the disk midplane temperature, Tdisk, panel (c) the optical depth, τ, and panel (d) the mass flux flux. The thin vertical lines in panel (a) indicate the respective position of rc. The horizontal lines in panel (b) indicate the ambient temperature Tamb = 20 K. The horizontal dashed lines in panel (c) symbolize τ = 1, dividing optically thin regions (τ ≪ 1) from optically thick regions (τ ≫ 1).

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