All Tables

Table 1: Overview of model parameters. From left to right, the columns indicate: planet mass in ${{M}_\oplus }$ , value of the adiabatic exponent ( $\Gamma =1$ means a locally isothermal equation of state), viscosity parameter $\alpha$ , radiation flag, accretion flag and the number of refinement levels. When $n_{\rm lev}$ levels of refinement are used, the local resolution within a distance of 2H from the planet is a factor $2^{n_{\rm lev}}$ higher than the base resolution of $\Delta r=0.0082~r_{\rm p}$ . For the local models, the indicated resolution is valid for the whole computational domain.