Table A.1.
Summary of the new direct N-body evolutionary models of star clusters and their GR-merger yields in this work.
| No. | Mcl/Msamp | rh/pc | W0 | Z | fbin | Tevol/Myr | remnant model | SN kick | BH spin | Nmrg, in | Nmrg, out |
|---|---|---|---|---|---|---|---|---|---|---|---|
| 1 | 17.5 × 104 | 2.0 | 7.0 | 0.0002 | 0.052 | 300.0 | rapid+B16 | mom. cons.3 | FM194 | 0 | 3 |
| 2 | 0 | 1 | |||||||||
| 3 | 0 | 1 | |||||||||
| 4 | 2 | 2 | |||||||||
| 5 | 7.5 × 104 | 2.0 | 7.0 | 0.001 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 1 | 3 |
| 6 | 2 | 1 | |||||||||
| 7 | 0 | 1 | |||||||||
| 8 | 1 | 0 | |||||||||
| 9 | 7.5 × 104 | 2.0 | 7.0 | 0.005 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 0 | 1 |
| 10 | 0 | 0 | |||||||||
| 11 | 0 | 1 | |||||||||
| 12 | 0 | 0 | |||||||||
| 13 | 7.5 × 104 | 2.0 | 7.0 | 0.01 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 0 | 0 |
| 14 | 1 | 0 | |||||||||
| 15 | 0 | 0 | |||||||||
| 16 | 0 | 0 | |||||||||
| 17 | 7.5 × 104 | 2.0 | 7.0 | 0.02 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 0 | 1 |
| 18 | 0 | 0 | |||||||||
| 19 | 1 | 0 | |||||||||
| 20 | 0 | 0 | |||||||||
| 21 | 7.5 × 104 | 2.0 | 9.0 | 0.0002 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 1 | 2 |
| 22 | 2 | 3 | |||||||||
| 23 | 0 | 0 | |||||||||
| 24 | 0 | 1 | |||||||||
| 25 | 7.5 × 104 | 2.0 | 9.0 | 0.001 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 1 | 0 |
| 26 | 1 | 1 | |||||||||
| 27 | 0 | 1 | |||||||||
| 28 | 0 | 1 | |||||||||
| 29 | 7.5 × 104 | 2.0 | 9.0 | 0.005 | 0.05 | 300.0 | rapid+B16 | mom. cons. | FM19 | 2 | 1 |
| 30 | 1 | 1 | |||||||||
| 31 | 0 | 0 | |||||||||
| 32 | 1 | 1 | |||||||||
Notes.
The binary fraction is defined as fbin = 2Nbin/N, with Nbin being the total number of binaries and N being the total number of members. Notably, the initial binary fraction among the O stars, considered separately, is fObin = 1.0 as opposed to the smaller overall binary fraction, fbin.
Vanishing BH natal spins (Fuller & Ma 2019).
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