Table 2.
Values for the parameters describing the dark matter profiles (i.e. ρh, 0, the halo density; lh, 0, the typical halo scale length; and m, the halo index) as a function of the stellar mass M⋆.
| M⋆ | ρh, 0 | lh, 0 | m | MBH |
|---|---|---|---|---|
| log10([M⊙]) | [M⊙ pc−3] | [kpc] | log10([M⊙]) | |
| 9.5 | 3 × 10−4 | 20 | 3 | 5.5 |
| 10 | 6 × 10−4 | 25 | 3.5 | 6 |
| 10.5 | 7 × 10−4 | 30 | 1.5 | 6.5 |
| 11 | 8.5 × 10−4 | 35 | 2 | 7 |
Notes. Those values have been inspired by the work of Kun et al. (2017), but their final values have been chosen to match the PHANGS rotation curves. The central black hole masses MBH we use in the initial conditions are also shown in the last column.
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