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Table 4
Final fate of dynamical BBH mergers (model DynA) in HM clusters.
| IC | Ej3B | InCl | EjGR | Cl† | AfterDisr |
|---|---|---|---|---|---|
| (%) | (%) | (%) | ×10−3% | ×10−3% | |
| kro1 | 95.27 | 1.03 | 3.69 | 0.62 | 5.42 |
| lar1 | 97.09 | 0.68 | 2.23 | 0 | 1.02 |
| lar5che | 96.99 | 0.74 | 2.27 | 0 | 4.77 |
| log1 | 98.68 | 0.42 | 0.90 | 0 | 0 |
| log1che | 98.71 | 0.39 | 0.89 | 0 | 0 |
| top1 | 99.67 | 0.12 | 0.21 | 0 | 0 |
Notes. Same as Table 3, but for dynamical BBH mergers using the pairing criterion DynA. In this case, no BBH merger can have the EjSN flag because we assumed that the single BHs ejected by supernova kick no longer pairs up.
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