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Table 8.
Initial condition parameters of the simulations.
| Label | m2/m1 | M200, 1 | rs, 1 | c1 | M⋆, 1 | M200, 2 | rs, 2 | c2 | M⋆, 2 |
|---|---|---|---|---|---|---|---|---|---|
| (M⊙) | (kpc) | (M⊙) | (M⊙) | (kpc) | (M⊙) | ||||
| S1 | 0.1 | 1.00 × 1012 | 26.3 | 7.9 | 2.73 × 1011 | 1.00 × 1011 | 9.8 | 9.8 | 2.73 × 1010 |
| S3 | 0.3 | 8.46 × 1011 | 24.4 | 8.0 | 2.31 × 1011 | 2.54 × 1011 | 14.6 | 9.0 | 6.92 × 1010 |
| S5 | 0.5 | 7.33 × 1011 | 23.0 | 8.1 | 2.00 × 1011 | 3.67 × 1011 | 17.1 | 8.7 | 1.00 × 1011 |
| S7 | 0.7 | 6.47 × 1011 | 21.8 | 8.2 | 1.76 × 1011 | 4.53 × 1011 | 18.7 | 8.5 | 1.24 × 1011 |
| S9 | 0.9 | 5.79 × 1011 | 20.8 | 8.3 | 1.58 × 1011 | 5.21 × 1011 | 19.8 | 8.4 | 1.42 × 1011 |
Notes. Each model has a different mass ratio and the following values are given for the primary galaxy (subscript 1) and the secondary galaxy (subscript 2): virial mass, NFW scale length, concentration and stellar mass.
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