Fig. 1
Density and dust temperature structures in the inner 200 AU radius for all three simulations at t ~ 1.2 × 105 years. Temperature contours at 25 K and 40 K are indicated in the right panels. Top: a vertical slice (R − z slice at φ = 0 where R denotes the cylindrical radial coordinate) of the 3D MHD simulation of RSD formation. Middle: a vertical slice of the 3D MHD simulation of a pseudo-disk (no RSD). Bottom: 2D semi-analytical disk formation model. The red lines highlight the region of the stable RSD.
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