50 citations · 155 across the 12 of their papers we have counts for
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astro-ph.EP2024★ 10 cited
Using the helium triplet as a tracer of the physics of giant planet outflows
Matthäus Schulik, James Owen
Hydrodynamic outflows, such as those observed escaping close-in gas giant planets, are not isothermal in structure. Their highly ionized nature allows them to cool adiabatically at…
astro-ph.EP2024★ 1 cited
Gas dynamics around a Jupiter-mass planet I. Influence of protoplanetary disk properties
E. Lega, M. Benisty, A. Cridland +3
Giant planets grow and acquire their gas envelope during the disk phase. At the time of the discovery of giant planets in their host disk, it is important to understand the interpl…
astro-ph.EP2024★ 7 cited
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, . However, the…