Table 3
Summary of the runs.
Model | nS | ΔS | t1 | t2 | t3 | ΔB | Ωp | ωI |
|
||||||||
B-0 | – | – | 0.75 | 1.4 | 2.2 | – | 49 | 2.9 |
B-1 | 1 | – | 0.75 | 1.2 | 1.8 | –200 | 48 | 3.0 |
B-1m | 1 | – | 0.75 | 2 | 2.4 | 300 | 49 | 2.9 |
B-4 | 4 | – | 0.75 | 1.3 | 2.0 | –300 | 49 | 2.9 |
B-4m | 4 | – | 0.75 | 1.7 | 2.5 | 470 | 48 | 3.0 |
B-23 | 23 | – | 0.75 | 1.1 | 1.7 | –310 | 48 | 2.9 |
B-1-110 | 1 | +110 | 0.75 | 1.6 | 2.5 | 600 | 48 | 2.9 |
B-1-500 | 1 | –500 | 0.40 | 1.0 | 2.2 | –20 | 48 | 2.7 |
Notes. nS is the number of satellites; “m” denotes only mass-rescaled satellites while the remaining simulations are fully – mass, positions and velocities – rescaled. t1, t2, t3 denote the times (in Gyr) of the jump, the onset and the end of the exponential growth of the bar, respectively. ΔB is the delay of the bar growth in Myr with respect to the isolated case B-0. Pattern speed Ωp in km s-1 and exponential growth rate ωI in Gyr-1 are given in the last columns.
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