Blowin' in the non-isothermal wind: core-powered mass loss with hydrodynamic radiative transfer

William Misener, Matthäus Schulik, Hilke E. Schlichting +1

The mass loss rates of planets undergoing core-powered escape are usually modeled using an isothermal Parker-type wind at the equilibrium temperature, $T_{\mathrm{eq}}$. However, the…