November 10, 2020 (v1)
Publication
It is well known that giant planets open deep gaps in their natal gaseous protoplanetary discs. However, it is unclear how gas accretion onto growing planets influences the shape and depth of their growing gaps. We perform isothermal hydrodynamical simulations with the Fargo-2D1D code in which planets accrete gas within full discs that range...
Uploaded on: December 4, 2022