Open Access
Table B.1
Remaining binary populations at 500 Myr.
| Model ID | K0.0 | K0.6 | K1.2 | K1.8 | NOK0.0 | NOK0.6 | NOK1.2 | NOK1.8 |
|---|---|---|---|---|---|---|---|---|
| nb | 355 ± 19 | 356 ± 19 | 390 ± 20 | 313 ± 18 | 358 ± 19 | 400 ± 20 | 350 ± 19 | 315 ± 18 |
| ncb | 220 ± 15 | 212 ± 15 | 250 ± 16 | 195 ± 14 | 228 ± 15 | 263 ± 16 | 214 ± 15 | 192 ± 14 |
| nBHBH | 98 ± 10 | 87 ± 9 | 113 ± 11 | 79 ± 9 | 104 ± 10 | 112 ± 11 | 85 ± 9 | 80 ± 9 |
| nBHstar | 106 ± 10 | 111 ± 11 | 118 ± 11 | 101 ± 10 | 109 ± 10 | 129 ± 11 | 117 ± 11 | 98 ± 10 |
| nNSb | 16 ± 4 | 14 ± 4 | 19 ± 4 | 15 ± 4 | 15 ± 4 | 22 ± 5 | 12±3 | 14 ± 4 |
Notes. Columns list the eight NBODY6++GPU simulations. Rows give the numbers of remaining binaries nb, compact binaries ncb, BHBH binaries nBHBH, binaries containing a BH and a non-compact star nBHstar, and NS binaries nNSb. Notes on the uncertainty are given in Appendix B.
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