Table 2.
Example solutions of allowed IMBH parameters that do not disrupt the S-star cluster in 1 Myr.
| Parameter | IMBHi1 | IMBHi2 | IMBHi3 | IMBHo1 |
|---|---|---|---|---|
| Mi (M⊙) | 1282 | 1321 | 1130 | 3226 |
| ai (″) | 0.032 | 0.033 | 0.075 | 0.435 |
| ei | 0.73 | 0.69 | 0.49 | 0.56 |
| ii (°) | 52.29 | 63.85 | 75.31 | 274.03 |
| Ωi (°) | 155.42 | 161.59 | 291.45 | 95.95 |
| ωi (°) | 195.74 | 171.54 | 156.02 | 180.71 |
Notes. The IMBHi1–IMBHi3 solutions lie inside the S2 orbit, while IMBHo1 is outside.
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