Upper panel: disk scale height (H∕R, solid lines) as a function of radius for the different planetary masses, 5 M_⊕ (blue) and 10 M_⊕ (red), for themodels with radiative transfer. The purple dotted lines at 0.05 and 0.02 represent the H∕R of the isothermal simulations performed, respectively. Lower panel: midplane gas temperature (T, solid lines) for the corresponding models as on the top panel. The black dashed line represents the initial temperature.