Fig. 14
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Gas surface density (hundred times of the dust; top) and effective turbulence strength for the disk gas accretion (bottom) estimated from our fiducial active disk models. The gray dashed line denotes the gas surface density of the minimum mass solar nebula (MMSN; Hayashi 1981). The dotted lines denote the criteria for the disk to be gravitation-ally unstable (Q = 1).
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