Table 3.
Structural and orbital parameters of the clusters resulting from the mergers at the end of the simulation (12 Gyr).
| ID | Mf (M⊙) | Mf, 1 (M⊙) | Mf, 2 (M⊙) | rc (pc) | rh (pc) | rt (pc) | b/a|c | c/a|c | e | rp (kpc) | ra (kpc) |
|---|---|---|---|---|---|---|---|---|---|---|---|
| CM1 | 9.4 × 106 | 4.7 × 106 | 4.7 × 106 | 1.0 | 9.5 | 82 | 0.85 | 0.84 | 0.7 | 0.68 | 6.9 |
| CM2 | 5.1 × 106 | 2.6 × 106 | 2.5 × 106 | 2.2 | 7.3 | 114 | 0.97 | 0.84 | 0.9 | 0.12 | 1.84 |
| CM12 | 8.9 × 106 | 8.0 × 106 | 9.3 × 105 | 1.4 | 4.7 | 99 | 0.95 | 0.74 | 0.6 | 0.17 | 2.2 |
Notes. The final mass of the clusters (Mf) and the mass belonging to each of the progenitors (Mf, 1 and Mf, 2) are listed together with the core, half-mass, and tidal radii (rc, rh and rt). The axial ratios at the core radius (b/a|c and c/a|c) and the eccentricity (e), perigalacticon (rp) and apogalacticon (ra) are also shown.
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