Table 1
Parameters and initial conditions of the simulations.
| Model | α A | α D | Mdisk [M⊙] | uf [m s-1] | rdz [AU] | E d |
|
|
||||||
| A2 | 10-2 | 10-2 | 0.20 | 3.0 | – | 1.0 |
| A3 | 10-3 | 10-3 | 0.20 | 3.0 | – | 1.0 |
| A4 | 10-4 | 10-4 | 0.20 | 3.0 | – | 1.0 |
| A5 | 10-5 | 10-5 | 0.20 | 3.0 | – | 1.0 |
| D23_M05 | 10-2 | 10-3 | 0.05 | 3.0 | 35 | 1.0 |
| D25_M05 | 10-2 | 10-5 | 0.05 | 3.0 | 35 | 1.0 |
| D35_M05 | 10-3 | 10-5 | 0.05 | 3.0 | 35 | 1.0 |
| LDE | 10-2 | 10-5 | 0.05 | 3.0 | 35 | 0.1 |
| COAG | 10-5 | 10-5 | 0.20 | − | – | 0.0 |
Notes. Models A2 through A5 are the completely active disks, models starting with D are the disks with dead zones, LDE stands for low drift efficiency, and COAG is a model with neither radial drift nor fragmentation. Other relevant initial conditions are the stellar mass M ⋆ = 1 M⊙, stellar temperature T ⋆ = 4300 K, and R ⋆ = 2.5 R⊙.
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