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Fig. 3

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Cuts through the temperature distributions derived by the MCRT (left column) and RHD simulations (central column) and their relative differences δT (right column). The upper and lower rows show results for the midplane and a vertical cut through it at the azimuthal position of the planet, respectively. The color bar for the temperature distributions (relative differences) is displayed above (to the right). Additionally, the high-resolution and the low-resolution regions are divided by a green-gray line that is shown in the plots of the RHD simulations (i.e., in the central column). Here, the high-resolution (low-resolution) region is located on the green (gray) side of the line.

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