Table 4
Fractions of discs influenced by encounters.
| Model |
|
freduced | f< 1000 AU | f< 100 AU | fdestroyed | |
| [ pc-3] | ||||||
|
|
||||||
| D0 | 15 | 65.1% | 42.8% | 8.8% | 3.4% | |
| D1 | 30 | 75.4% | 53.7% | 11.0% | 3.7% | |
| D2 | 61 | 82.7% | 64.9% | 14.6% | 4.3% | |
| D3 | 122 | 87.1% | 74.2% | 20.4% | 5.2% | |
| D4 | 245 | 89.2% | 81.3% | 28.8% | 6.4% | |
| D5 | 489 | 88.7% | 83.9% | 39.2% | 8.7% | |
Notes. Fraction of stars with disc-size-reducing encounters (Col. 3), with discs smaller than 1000 AU (Col. 4), with discs smaller than 100 AU (Col. 5), and with destroyed discs (Col. 6) in the different cluster models (Col. 1) after 5 Myr of cluster evolution. The average number densities of the cluster models are given in Col. 2 (rounded values, taken from Table 3).
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