Table 2
Table of runs.
| Model | γF | Md | D | si |
| label | [degrees] | [ ] |
[AU] | [m] |
|
|
||||
| 1 | 0 | 1 | 60 | 10 000 |
| 2 | 25 | 1 | 60 | 10 000 |
| 3 | 45 | 1 | 60 | 10 000 |
| 45 | 1 | 60 | 1000 | |
| 45 | 1 | 60 | 100 | |
| 4 | 45 | 3 | 60 | 10 000 |
| 5 | 45 | 6 | 60 | 10 000 |
| 6 | 45 | 1 | 90 | 10 000 |
| 7 | 45 | 1 | 120 | 10 000 |
| 8 | 25 | 1 | 60 | 100 |
| 25 | 1 | 60 | 1000 | |
| 25 | 1 | 60 | 10 000 | |
| 9 | 45 | 1 | 60 | 100 |
| 45 | 1 | 60 | 1000 | |
| 45 | 1 | 60 | 10 000 | |
Notes. The first column gives the run label; the second column gives the inclination of the binary companion to the gas-plus-planetesimal disc, γF; the third column gives the disc mass in units of the reference mass; the fourth column gives the binary separation, D; the fifth column lists the planetesimal radii, si, included in the models.
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