Table 1.
Initial conditions for the cooling isolated halo.
| Mhalo | c200 | R200 | T200 | Zavg | nSF | M* | ϵSN | Δxmax |
|---|---|---|---|---|---|---|---|---|
| (in M⊙) | (in kpc) | (in K) | (in Z⊙) | (in H cm−3) | (in M⊙) | (in pc) | ||
| 1011 | 3.4 | 42.82 | 3.6 × 105 | 0.3 | 10 | 104 | 0.2 | 12 |
Notes. From left to right: halo mass (Mhalo), NFW concentration (c200), virial radius (R200), virial temperature (T200), average metallicity (Zavg), density threshold for star formation (nSF), stellar mass resolution (M*), SN feedback efficiency (ϵSN) and smallest cell size (Δxmax).
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