Table 3
Primary galaxy–cluster interaction simulations performed in this work.
| Run | Cluster | Galaxy | b | max v | max ρ ICM |
| label |
|
|
|
||
|
|
|||||
| S1 | A | G1a | 100 | 3151 | 6.4 × 10-27 |
| S2 | A inc | G1a | 100 | 3141 | 6.3 × 10-27 |
| S3 | B | G1a | 500 | 1719 | 1.5 × 10-28 |
| S4 | C | G1a | 100 | 1255 | 2.6 × 10-27 |
| S5 | A | G2 | 100 | 3173 | 6.4 × 10-27 |
| S6 | B | G2 | 500 | 1780 | 1.7 × 10-28 |
| S7 | C | G2 | 100 | 1265 | 2.7 × 10-27 |
Notes.The initial impact parameter b is chosen for trajectories as if galaxy and cluster were point masses; the value actually obtained in the self-consistent simulation (see Fig. 2a) is different. Run S2 is identical to run S1, except that the galaxy is rotated by 90°, resulting in a different effective inclination throughout the orbital path (see Fig. 2c).
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