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Table 1

Estimates of turbulent α in our models.

h Mp
0.10 4.51 × 10−4 0.115 2.53 × 10−4 0.103
0.10 0.3 8.39 × 10−4 0.058 1.40 × 10−4 0.045
0.05 1.82 × 10−4 0.128 1.06 × 10−4 0.117
0.05 2.4 1.32 × 10−3 0.056 4.21 × 10−5 0.039

Notes. Planet mass is quoted in Mth. Values for models with embedded planets serve as upper limits, especially for the last model where the VSI is only present in in the inner disk (see Fig. 9).

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