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Table 3.
Dwarf galaxies simulated with the zoom-in technique.
| Model | LV | M⋆ | M200 | SF Class |
|---|---|---|---|---|
| ID | [106 L⊙] | [106 M⊙] | [109 M⊙] | |
| h050 | 4.2 | 9.6 | 2.6 | Extended |
| h070 | 2.0 | 5.8 | 1.8 | Extended |
| h061 | 0.2 | 0.5 | 1.9 | Quenched |
| h141 | 0.2 | 0.6 | 0.8 | Quenched |
| h111 | 0.2 | 0.5 | 1.1 | Quenched |
| h122 | 0.1 | 0.4 | 1.0 | Quenched |
| h159 | 0.4 | 1.1 | 0.7 | Quenched |
| h168 | 0.1 | 0.3 | 0.6 | Quenched |
| h177 | 0.2 | 0.5 | 0.5 | Quenched |
Notes. For each of them we provide the total V-band luminosity LV, total stellar mass M⋆, virial mass M200, and the star formation type for the unperturbed models at z = 0.
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