From top to bottom: azimuthally averaged gas density, gas pressure, and gas temperature. From left to right: NOWIND model, PEWIND model, and their relative difference. Dashed white lines are density contours for (from top to bottom) 10⁻¹⁷ to 10⁻¹³ g cm⁻³ in increments of one order of magnitude. Dotted red lines are column density contours for (from top to bottom) 2.5 × 10²⁰, 2.5 × 10²¹, and 2.5 × 10²² cm⁻². The arrows in the second row represent the pressure gradient force. In the right column, only the contours of the PEWIND model are shown. The white circles indicate the extent of the planet’s Hill sphere.