Fig. 8.

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Slices through the center of the domain for runs G1, G2, G3, and G4 (respectively first, second, third, and fourth columns) showing the local radiative flux in a top-down (top row, panels a–d) and edge-on (bottom row, panels e–h) view. The slices illustrate the structure of the accretion shock as well as the presence of spirals in the inner disk (see Eq. (1)). The scale bar in panels d and h apply to all other panels as well. The slices are shown at a moment in time where the inner disks have reached a radius of ≈0.5 AU. The mass of each inner disk is displayed in the top-right corners of panels a–d.
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