Table 3
Final fate of original BBH mergers in HM clusters.
| IC | Ej3B | EjSN | InCl | EjGR | Cl† | AfterDisr |
|---|---|---|---|---|---|---|
| (%) | (%) | (%) | (%) | ×10−3% | ×10−3% | |
| kro1 | 96.98 | 2.36 | 0.11 | 0.54 | 0 | 1.75 |
| kro5 | 92.59 | 0.14 | 1.72 | 5.55 | 0 | 0 |
| lar1 | 97.33 | 1.96 | 0.12 | 0.58 | 0.60 | 0.60 |
| lar5 | 93.37 | 0.09 | 1.71 | 4.82 | 2 | 0 |
| lar5che | 83.55 | 0 | 3.01 | 13.42 | 2.31 | 9.25 |
| log1 | 98.36 | 1.33 | 0.12 | 0.19 | 0 | 0 |
| log1che | 97.75 | 1.51 | 0.18 | 0.56 | 0.45 | 0 |
| log2 | 99.84 | 0.04 | 0.06 | 0.06 | 0 | 0 |
| log3 | 98.23 | 1.22 | 0.48 | 0.07 | 2.65 | 0 |
| log4 | 98.18 | 1.09 | 0.30 | 0.43 | 0 | 0 |
| log5 | 99.84 | 0.04 | 0.06 | 0.06 | 0 | 0 |
| top1 | 99.18 | 0.80 | 0.02 | 0.01 | 0 | 0 |
| top5 | 99.96 | 0.01 | 0.01 | 0.02 | 0 | 0 |
Notes. The first column reports all the considered initial conditions, and the following columns contain the percentages of BBH mergers with a specific flag from FASTCLUSTER . Ej3B means that the systems was ejected by three-body encounters; EjSN stands for binary systems that were ejected from the cluster by a supernova kick; InCl means that the BBH merger occurred inside the cluster and that its remnant remains inside the cluster; EjGR denotes systems that merge inside the cluster whose remnant is kicked outside of it because of the relativistic kick; Cl† represents the BBHs that merge outside the cluster after its evaporation; and finally, AfterDisr describes the percentage of BBHs that merge at z < zmin, with zmin = 2.
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