Giant planets with large metal masses and metal fractions such as HD 149026b and TOI-849b form via giant impacts in a rapidly dissipating disk by photoevaporation
06-11-2021
Formation & evolution, System architectures and dynamics, Planet interiors, Atmospheric characterization
giant planets; photoevaporation; giant impacts;
Gijs Mulders
Why do small stars have all the exoplanets?
02-11-2021
Formation & evolution, System architectures and dynamics