Table 1.
Initial parameters of the host and the satellite models used in the N-body simulations.
| Host | Sat. comp. | Sat. intermed. | Sat. ext. | |
|---|---|---|---|---|
| M200/M⊙ | 1.2 × 1012 | 1010 | 109 − 1010 | 1010 |
| Np | 2 × 106 | 1.3 × 104 | 1.3–13 × 103 | 1.3 × 103 |
| rs[kpc] | 15 | 0.5 | 3 | 10 |
| r1/2[kpc] | 20 | 1.5 | 5.5 | 18 |
| M1/2/M⊙ | 6 × 1012 | 5 × 1011 | 0.5–5 × 1011 | 5 × 1011 |
| Rtr [kpc] | 200 | 1 | 5 | 25 |
| ϵ [kpc] | 0.3 | 0.3 | 0.2–0.4 | 0.6 |
Notes. The satellite models include rigid, compact live (globular cluster type), intermediate live (dwarf galaxy type), and extended live (early type). From top to the bottom: Total mass (M200), the number of particles (Np), the scale radius (rs) of the NFW density profile, the half mass radius and half mass (r1/2, M1/2), the truncation radius (Rtr), and the smoothing length (ϵ). For rigid satellite M200/M⊙ = 1 × 1010, ϵ = 0.6 kpc.
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