Table 2.
Percentage of peculiar events in YSCs, GCs, and NSCs.
| Event |
 |
 |
 |
|---|---|---|---|
| Merger | 0.2 | 2.4 | 11.8 |
| Merger tcoal < 1 Myr | 14.8 | 4.6 | 4.0 |
| PIBH | 44.3 | 33.3 | 27.7 |
| IMBH | 1.6 | 0.7 | 0.4 |
| Merger with e10 Hz > 0.1 | 1.6 | 1 | 0.6 |
| Merger with e1 Hz > 0.1 | 9 | 1.8 | 0.9 |
| Retained BH remnants | 0 | 3.1 | 19.9 |
Notes. Line 1: percentage of BBH mergers over all the three-body simulations. Line 2: percentage of BBH mergers that take place during the three-body simulation with ARWV over all the BBH mergers. Line 3: percentage of pair-instability BHs produced by the merger. Line 4: percentage of intermediate-mass BHs (IMBHs) produced by the merger. Line 5: percentage of BBH mergers with an eccentricity at a GW frequency of 10 Hz e10 Hz > 0.1 with respect to all BBH mergers. Line 6: percentage of BBH mergers with an eccentricity at a GW frequency of 1 Hz e1 Hz > 0.1 with respect to all BBH mergers. Line 7: percentage of BHs produced by BBH mergers that happen before star cluster evaporation and are retained inside the cluster after the three-body interaction and the GW recoil.
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