Table 1
Simulation parameters.
| Name | B0 | mp [mJ] | h0 | K0 |
|---|---|---|---|---|
| L-m1-h03 | 0.046 | 1 | 0.03 | 4.12 · 104 |
| L-m1-h036 | 0.046 | 1 | 0.036 | 1.65 · 104 |
| L-m1-h04 | 0.046 | 1 | 0.04 | 9.77 · 103 |
| L-m1-h045 | 0.046 | 1 | 0.045 | 5.42 · 103 |
| L-m1-h05 | 0.046 | 1 | 0.05 | 3.20 · 103 |
| L-m1-h055 | 0.046 | 1 | 0.055 | 1.99 · 103 |
| L-m1-h06 | 0.046 | 1 | 0.06 | 1.29 · 103 |
| L-m1-h065 | 0.046 | 1 | 0.065 | 8.62 · 102 |
| L-m3-h036 | 0.046 | 3 | 0.036 | 1.49 · 105 |
| L-m3-h05 | 0.046 | 3 | 0.05 | 2.88 · 105 |
| L-m3-h06 | 0.046 | 3 | 0.06 | 1.16 · 105 |
| L-m13-h036 | 0.046 | 13 | 0.036 | 2.9 · 106 |
| L-m13-h06 | 0.046 | 13 | 0.06 | 2.17 · 105 |
| L-m13-h1 | 0.046 | 13 | 0.1 | 1.69 · 104 |
| M-m1-h03 | 0.15 | 1 | 0.03 | 4.12 · 104 |
| M-m1-h036 | 0.15 | 1 | 0.036 | 1.65 · 104 |
| M-m1-h04 | 0.15 | 1 | 0.04 | 9.77 · 103 |
| M-m1-h045 | 0.15 | 1 | 0.045 | 5.42 · 103 |
| M-m1-h05 | 0.15 | 1 | 0.05 | 3.20 · 103 |
| M-m1-h055 | 0.15 | 1 | 0.055 | 1.99 · 103 |
| M-m1-h06 | 0.15 | 1 | 0.06 | 1.29 · 103 |
| M-m1-h065 | 0.15 | 1 | 0.065 | 8.62 · 102 |
| M-m3-h036 | 0.15 | 3 | 0.036 | 1.49 · 105 |
| M-m3-h05 | 0.15 | 3 | 0.05 | 2.88 · 105 |
| M-m3-h06 | 0.15 | 3 | 0.06 | 1.16 · 105 |
| M-m13-h036 | 0.15 | 13 | 0.036 | 2.9 · 106 |
| M-m13-h06 | 0.15 | 13 | 0.06 | 2.17 · 105 |
| M-m13-h1 | 0.15 | 13 | 0.1 | 1.69 · 104 |
Notes. The simulations are named according to the following rules: “L” or “M” to indicate a light or massive disk, respectively; “m” followed by a number to indicate the planet mass (measured in Jupiter masses); “h” followed by a number to indicate the aspect ratio. B0 and K0 = q2/(αh5) are the disk-to-planet mass ratio and the gap depth parameter both evaluated at the initial planet location. The table contains all the simulations used in this work (both the new ones and those already presented in Scardoni et al. 2022).
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