Table 1
Table of all simulations.
| Name | Simulation | (Nr,Nϑ,Nϕ) | η = Mp/M ⋆ | r p | r domain | ϑ domain (dϑ) | ϕ domain | h/r | SF | |
| [AU] | [AU] | [rad] | [rad] | |||||||
|
|
||||||||||
| S1 | HD | (256,128,256) | no planet | – | [1,10] | 0.3 | 2π | 0.07 | unperturbed | |
| SP4 | HD | (256,128,256) | 10-4 | 5.0 | [1,10] | 0.3 | 2π | 0.07 | gap | |
| SP1 | HD | (256,128,256) | 10-3 | 5.0 | [1,10] | 0.3 | 2π | 0.07 | gap | |
|
|
||||||||||
| ST1 | MHD | (256,128,256) | no planet | – | [1,10] | 0.3 | 2π | 0.07 | zonal flow | |
| SPT4 | MHD | (256,128,256) | 10-4 | 5.0 | [1,10] | 0.3 | 2π | 0.07 | p.gap | |
| SPT6 | MHD | (256,128,256) | 10-3 | 5.0 | [1,10] | 0.3 | 2π | 0.07 | gap | |
Notes. In the last column, SF refers to “special feature” and the terms have the following meaning. p.gap means partial gap, gap means full gap and zonal flow means that there are magnetic field induced density bumps in the disk. The hydrodynamical simulations are characterized as HD and the magnetohydrodynamical ones as MHD. The name gives the link to the density maps shown in Fig. 1.
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