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Table 1.

Summary of simulations, including key results.

Run Gas distribution Cooling? LAGN vout out p ˙ out c / L AGN $ \dot{p}_{\mathrm{out}} c/L_{\mathrm{AGN}} $ E ˙ k , out / L AGN $ \dot{E}_{\mathrm{k, out}}/L_{\mathrm{AGN}} $
(erg s−1) (km s−1) (M yr−1) (×10−3)
SmthAdiaL0.3 Smooth No 3.78 × 1045 350 642 (348) 11.3 (6.1) 7.64 (4.14)
SmthAdiaL1.0 Smooth No 1.26 × 1046 582 966 (671) 8.44 (5.86) 9.34 (6.49)
SmthCoolL0.3 Smooth Yes 3.78 × 1045 96.2 229 (166) 1.1 (0.8) 0.20 (0.15)
SmthCoolL1.0 Smooth Yes 1.26 × 1046 304 485 (402) 2.21 (1.83) 1.23 (1.02)
TurbAdiaL0.3 Turbulent No 3.78 × 1045 312 641 (313) 10 (4.89) 8.70 (4.26)
TurbAdiaL1.0 Turbulent No 1.26 × 1046 556 1030 (630) 8.64 (5.26) 11.22 (6.83)
TurbCoolL0.3 Turbulent Yes 3.78 × 1045 140 116 (23.3) 0.817 (0.164) 0.78 (0.16)
TurbCoolL1.0 Turbulent Yes 1.26 × 1046 297 710 (309) 3.18 (1.38) 3.38 (1.47)

Analytical-L0.3 3.78 × 1045 590 − 790 565 − 760 17 − 30 0.016 − 0.04
Analytical-L1.0 1.26 × 1046 885 − 1180 850 − 1130 11 − 20 0.017 − 0.039

Notes. The first column shows the simulation name, the second – the type of gas distribution used, the third – the presence or absence of radiative cooling, and the fourth shows the AGN luminosity. The subsequent columns show the results: mass-weighted outflow velocity, time-averaged mass outflow rate, and momentum and energy loading factors. In the final three columns, the first value is evaluated assuming τ = τAGN, while the one in parentheses assumes τ = τr/v. All results evaluated at t = 0.5 Myr (see the main text for the reasoning). Two rows at the bottom show the analytical predictions for the main results, based on Zubovas & King (2012a). The lower velocity is that of the contact discontinuity, while the higher corresponds to the outer shock; other parameter ranges correspond to these two velocities.

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