Open Access

Fig. 15

image

HY-RTi run at t~0.7τff. Left panel: density slice perpendicular to the disk in a (10 000 AU)2 region. Right panel: scatter plot of the M1 radiative energy against the radius. Contours show the AMR level. The cavity edges are zones of primary absorption for the stellar radiation and are resolved to the highest level (12).

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