Table 2
Parameters related to the identification of binary systems that involve the MMO in each simulation.
| Simulation | Nbound | γmin 2 | M (γmin) 3 (M⊙) | MMMO 4 (M⊙) | a/aHS 5 |
|---|---|---|---|---|---|
| E1_1 | 0 | — | — | 462 | — |
| E1_2 | 2 | 1.88 | 232 | 439 | 18.28 |
| E1_3 | 2 | 7.53 | 292 | 420 | 66.68 |
| E2_1 | 8 | 0.037 | 754 | 1000 | 0.80 |
| E2_2 | 6 | 0.83 | 329 | 591 | 4.60 |
| E2_3 | 3 | 44.50 | 98 | 681 | 27.17 |
| E3_1 | 43 | 1.19 | 226 | 3950 | 1.64 |
| E3_2 | 1 | 2255 | 29 | 532 | 366.99 |
| E3_3 | 19 | 0.116 | 251 | 2317 | 0.31 |
| E6_1 | 34 | 0.009 | 335 | 4727 | 0.09 |
| E6_2 | 30 | 0.003 | 231 | 4699 | 0.03 |
| E6_3 | 40 | 0.92 | 231 | 4685 | 0.57 |
Notes. (1)Number of stars that are gravitationally bound to the MMO. (2)Minimum value of the perturbation parameter γmin among the bound stars, as defined in Eq. (20). (3)Mass of the star for which γ = γmin. (4)Mass of the MMO. (5)Ratio of the binary semimajor axis to the semimajor axis at the hard-soft boundary.
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