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Fig. 2.

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Azimuthally averaged surface density (top left), rotation rate (top right), poloidal magnetic field intensity (bottom left), and plasma parameter βP (bottom right) versus the radius, computed in the midplane. Each color corresponds to one snapshot, the darker being the disk formation epoch, while the lighter is associated with the later times of the simulation. In the top right panel, the dashed black line is the theoretical Keplerian rotation rate with M ≈ 0.7 M.

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