Fig. 7.
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Spacetime diagrams of the surface density (top panel), poloidal magnetic flux (middle panel), and Toomre parameter (bottom panel). Colors and radii are in log scale. The dashed white line corresponds to the disk radius, and dash-dotted white lines delimit the three accretion phases. Data were convolved in time using a 10 kyr window (equivalent to 8 orbits at 100 au).
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