Values of the subgrid parameters that vary between the models presented here. The parameters nH, 0 and nn control, respectively, the characteristic density and the power-law slope of the density dependence of the energy feedback from star formation (see equation 7 in Section 4.5.1). The parameter Cvisc controls the sensitivity of the BH accretion rate to the angular momentum of the gas (see equation 9 in Section 4.6.2) and ΔTAGN is the temperature increase of the gas during AGN feedback (see Section 4.6.4).
| Prefix . | nH, 0 . | nn . | Cvisc . | ΔTAGN . |
|---|---|---|---|---|
| . | (cm−3) . | . | . | (K) . |
| Ref | 0.67 | 2/ln 10 | 2π | 108.5 |
| Recal | 0.25 | 1/ln 10 | 2π × 103 | 109 |
| AGNdT9 | 0.67 | 2/ln 10 | 2π × 102 | 109 |
| Prefix . | nH, 0 . | nn . | Cvisc . | ΔTAGN . |
|---|---|---|---|---|
| . | (cm−3) . | . | . | (K) . |
| Ref | 0.67 | 2/ln 10 | 2π | 108.5 |
| Recal | 0.25 | 1/ln 10 | 2π × 103 | 109 |
| AGNdT9 | 0.67 | 2/ln 10 | 2π × 102 | 109 |
Values of the subgrid parameters that vary between the models presented here. The parameters nH, 0 and nn control, respectively, the characteristic density and the power-law slope of the density dependence of the energy feedback from star formation (see equation 7 in Section 4.5.1). The parameter Cvisc controls the sensitivity of the BH accretion rate to the angular momentum of the gas (see equation 9 in Section 4.6.2) and ΔTAGN is the temperature increase of the gas during AGN feedback (see Section 4.6.4).
| Prefix . | nH, 0 . | nn . | Cvisc . | ΔTAGN . |
|---|---|---|---|---|
| . | (cm−3) . | . | . | (K) . |
| Ref | 0.67 | 2/ln 10 | 2π | 108.5 |
| Recal | 0.25 | 1/ln 10 | 2π × 103 | 109 |
| AGNdT9 | 0.67 | 2/ln 10 | 2π × 102 | 109 |
| Prefix . | nH, 0 . | nn . | Cvisc . | ΔTAGN . |
|---|---|---|---|---|
| . | (cm−3) . | . | . | (K) . |
| Ref | 0.67 | 2/ln 10 | 2π | 108.5 |
| Recal | 0.25 | 1/ln 10 | 2π × 103 | 109 |
| AGNdT9 | 0.67 | 2/ln 10 | 2π × 102 | 109 |
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