Water-cooled (sub)-Neptunes get better gas mileage

Open Access

Fig. A.1.

Temperature profile (radial coordinate in units of planet radius) in a hydrodynamic flow for different lower boundary values H₂O/H₂ with a stellar EUV flux of $1000 F_{EUV}^{\oplus}$ $1000F_{\mathrm{EUV}}^{\oplus}$ , M_p = 5M_⊕, and g = 4 m s⁻², where $F_{EUV}^{\oplus}$ $F_{\mathrm{EUV}}^{\oplus}$ is the present EUV flux at Earth. Sonic points are marked by filled circles and the exobase is marked by triangles.

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