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Table 1
Simulation parameters and results.
| H/r | Nr | Ns | ν | T | XC | Ṁp |
( ) |
( ) |
(RH) | (MJup/yr) | |||
|
|
||||||
| 0.05 | 342 | 632 | 10-5 | −3.39 × 10-8 | 5.11 × 10-2 | 1.87 × 10-7 |
|
|
||||||
| 0.1 | 170 | 314 | 3 × 10-5 | −3.76 × 10-8 | 5.33 × 10-2 | 2.03 × 10-7 |
| 0.1 | 170 | 314 | 10-5 | −3.64 × 10-8 | 5.26 × 10-2 | 1.98 × 10-7 |
| 0.1 | 170 | 314 | 3 × 10-6 | −3.49 × 10-8 | 5.18 × 10-2 | 1.92 × 10-7 |
| 0.1 | 170 | 314 | 10-6 | −3.32 × 10-8 | 5.08 × 10-2 | 1.84 × 10-7 |
|
|
||||||
| 0.15 | 114 | 212 | 10-5 | −3.70 × 10-8 | 5.30 × 10-2 | 2.01 × 10-7 |
|
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| 0.2 | 86 | 160 | 3 × 10-5 | −3.88 × 10-8 | 5.40 × 10-2 | 2.09 × 10-7 |
| 0.2 | 86 | 160 | 10-5 | −4.02 × 10-8 | 5.47 × 10-2 | 2.15 × 10-7 |
Notes. Nr and Ns are the number of radial and azimuthal grid-cells respectively. ν is the viscosity, T the cumulated stellar torque, XC the equilibrium radius between the inner part of the disc in steady-state and the outer part. Finally, Ṁp is the accretion rate onto the planet.
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