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Fig. 3

image

Logarithmic density (left) and radial velocity (right) as a function of distance from the planet’s center for the isotropic outflow model used to initialize the 3D wind simulation for a “light” hot Jupiter (M° = 0.5 MJ, R° = 1.5 RJ). The symbols “+” and “×” denote, respectively, the high- and low-flux cases (modeled with T° = 104 K and T° = 6 × 103 K, respectively). The solid and dashed lines are from the corresponding 1D simulations that take into account the relevant heating and cooling processes (see text for details).

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