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Fig. B.1
Radial (top) and vertical (bottom) profile of the accretion stress α for three different resolutions and two different dust-to-gas mass ratios averaged over 200 inner orbits (300 to 500 inner orbits). Here, the cylindrical height Z is given by Z = Rmidsinθ with Rmid = 60 AU.
This figure is made of several images, please see below:
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