Table 1.
Configuration of the selected simulations.
| Simulation ID | V | ρ | Dead | Keplerian | r0 | r1 | Number of grids |
|---|---|---|---|---|---|---|---|
| factor | factor | zone? | rotation? | in AU | in AU | in radial direction | |
| Case A | −1.0 | 1.0 | No | No | 0.016 | 0.020 | 2 |
| Case B | −1.5 | 1.5 | No | No | 0.016 | 0.020 | 2 |
| Case C | −1.5 | 5.0 | No | No | 0.016 | 0.020 | 2 |
| Case D | −2.0 | 10.0 | No | No | 0.016 | 0.020 | 2 |
| Case C.1 | −1.5 | 5.0 | Yes | Yes | 0.016 | 0.020 | 2 |
| Case D.1 | −2.0 | 10.0 | Yes | Yes | 0.016 | 0.020 | 2 |
| Case C.2 | −1.5 | 5.0 | Yes | Yes | 0.012 | 0.018 | 3 |
| Case D.2 | −2.0 | 10.0 | Yes | Yes | 0.012 | 0.018 | 3 |
Notes. The simulations are identified in the first column, followed by the initial multiplying factors imposed for velocity (V) and density (ρ) with respect to the analytical solution in region 2 of Fig. 1. Some simulations include a dead zone (Col. 4) and a Keplerian rotating disk (Col. 5). Columns 6 and 7 define the limits of the fixed zone. Depending on the starting radius, a different number of adjacent grids has been used in the radial direction (last column).
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