Midplane rotational structure for the run H2 (left), with |v|∕v_Kep as contours. The potential of run H2 is four times deeper than that of run C1, which is shown in Fig. 7. The gravitational smoothing length is marked with the blue dashed circle. It becomes evident that the deeper potential does not extend the CPD necessarily much closer to the planet, rather the contrary. As pressure support increases, the maximum rotational support drops below 90%. The physical extent of the strongly rotating gas remains similar to C1. Cylindrically averaged structures are shown with the temperature as contours (right). The observed flows are similar to the isothermal results presented in Tanigawa et al. (2012) and consistent with previous high-opacity results from Lambrechts et al. (2019).