Table 4.
Properties at z = 0 of the dwarf models evolved in the moving box simulations.
| Name | R200 [kpc] | M200 [108 M⊙] | M⋆ [106 M⊙] | LV [106 L⊙] | Cold Gas [106 M⊙] | Hot Gas [106 M⊙] |
|---|---|---|---|---|---|---|
| h159_iso | 19.4 | 5.37 | 1.08 | 0.43 | 0 | 9.05 |
| h159_sta | 11.3 | 1.06 | 2.47 | 1.04 | 0 | 0. |
| h159_rho | 15.2 | 2.56 | 2.61 | 1.78 | 1.34 | 1.00 |
| h159_tem | 14.1 | 2.05 | 1.00 | 0.40 | 0 | 0. |
| h070_iso | 26.3 | 13.3 | 5.72 | 2.04 | 0 | 20.6 |
| h070_sta | 14.5 | 2.22 | 18.5 | 10.9 | 6.32 | 4.61 |
| h070_rho | 20.3 | 6.09 | 23.8 | 14.9 | 6.23 | 6.93 |
| h070_tem | 17.3 | 3.76 | 5.42 | 1.92 | 0 | 0. |
Notes. The model names fit the one of the corresponding dwarf in Revaz & Jablonka (2018). R200 and M200 corresponds to the virial radius and mass respectively. LV is the final V-band luminosity. The cold gas is defined as the gas with a temperature lower than 1000 K while the hot one with a temperature above.
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