Logarithm of the gas surface density in non-isothermal simulations with α_DZ = 10⁻³ and α_MRI = 5 × 10⁻². The panels correspond to different planet-to-star mass ratios as marked by the labels. Each planet is held in a fixed circular orbit with a_p = 0.12au. We overplot streamlines of the gas flow relative to the planet with white curves. The figure is also available as an online movie that scans all values of a_p for which the static torque was measured. Corresponding torque measurements can be found in the top row of Fig. 12 (blue data points).