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Table A.2.
Additional moving box simulations performed.
Model | M200 [108 M⊙] | M⋆ [106 M⊙] | LV [106 L⊙] | Cold gas [106 M⊙] | Hot gas [106 M⊙] |
---|---|---|---|---|---|
h050_sta | 8.8 | 117.34 | 17.63 | 14.10 | 103.2 |
h050_iso | 11.4 | 36.09 | 7.90 | 14.67 | 21.4 |
h123_tem | 3.4 | 2.78 | 0.14 | 0.00 | 2.8 |
h123_iso | 3.7 | 1.02 | 0.13 | 0.00 | 1.0 |
h132_rho | 6.1 | 77.33 | 17.85 | 12.44 | 64.9 |
h132_sta | 2.8 | 60.77 | 13.40 | 9.25 | 51.5 |
h132_tem | 5.0 | 24.52 | 9.08 | 11.24 | 13.3 |
h132_iso | 16.0 | 0.01 | 2.88 | 0.00 | 0.0 |
h168_tem | 8.5 | 4.54 | 1.09 | 0.00 | 4.5 |
h168_iso | 6.1 | 2.98 | 1.02 | 0.00 | 3.0 |
h074_rho | 2.6 | 34.01 | 2.57 | 3.84 | 30.2 |
h074_sta | 1.2 | 26.15 | 2.62 | 3.81 | 22.3 |
h074_tem | 2.4 | 9.41 | 2.34 | 3.64 | 5.8 |
h074_iso | 6.2 | 0.00 | 0.65 | 0.00 | 0.0 |
Notes. The Milky Way model is given with the model name following the same convention than in Table 3. The four last columns are the properties (total mass, luminosity, cold gas mass and hot gas mass) of the galaxies at the end of the simulation.
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