Fig. 14.
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Top-down (panel a) and edge-on (panel b) slices across the star-disk system showing the ratio of the wavelength of the most unstable MRI mode to cell size at the final snapshot of run NIMHD (t ≈ 0.55 yr after protostellar birth). The outer contour corresponds to the disk surface, whereas the inner one corresponds to the protostar’s surface.
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