Table 2
Properties of ejected fragments formed inside the disk.
| Model | Mfrag (MJup) | MHill (MJup) | vs (km s-1) | vi (km s-1) | Ekin/ | Egrav | |
|
|
|||||
| P1 | 24 | 45 | 1.67 | 2.20 | 3.32 (CM) |
| P2 | 21 | 40 | 1.18 | 2.80 | 2.93 (S) |
| P3 | 23 | 41 | 1.37 | 2.56 | 4.54 (S) |
| P4 | 25 | 44 | 1.46 | 1.65 | 1.75 (CM) |
| P6 | 10 | 23 | 1.88 | 2.15 | 2.92 (CM) |
| R1 | 10 | 25 | 2.13 | 3.33 | 7.32 (CM) |
Notes. Columns show, from left to right, the fragment mass Mfrag, the mass located inside the fragment’s Hill radius MHill, the velocity of the fragment relative to the disk central star vs and the intruder vi, and the ratio of kinetic to potential energy in the reference frame in which this ratio is the lowest with the reference frame indicated in brackets (CM = center of mass system, S = central star).
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