Table 6: Outflow properties of HzRGs.
Source $D_{\rm opt}$ $\Delta v$ $\tau_{\rm opt}$ $\dot{E}_{\rm kin,obs}$ $\dot{E}_{\rm kin,ext}$ $\dot{E}_{\rm shell}$

(1) (2) (3) (4) (5) (6) (7)

MRC0316-257 21 $\times$ 9 670 3.1 44.4

MRC0406-244 30 $\times$ 9 960 2.9 45.3 45.6 45.0

TXS0828+193 28 $\times$ 10 800 4.1 45.3 45.3 45.0

MRC1138-262 53 $\times$ 32 800 1 44.2 45.6

For comparison we add MRC1138-262 from Nesvadba et al. (2006b). Column (1) - source name. Column (2) - extent of the optical line emission in kpc along the major and minor axis, respectively. Column (3) - velocity offset between the blue and redshifted bubble in km s^-1 in the rest-frame. Column (4) - age of the outflow for constant $\Delta v$ and neglecting projection effects in 10⁷ yrs. Column (5) - energy injection necessary to power the outflow in erg s^-1 (``method 1'', see Sect. 5.5 for details), and mass estimates based on the measured H $\alpha$ fluxes, uncorrected for extinction. This serves as a strict lower limit to the kinetic energy injection. Column (6) - the same as Col. (5), but using extinction-corrected H $\alpha$ fluxes. Column (7) - energy injection necessary to inflate a hot bubble in erg s^-1 (``method 2'', see Sect. 5.5 for details).

**Table 6:** Outflow properties of HzRGs.
Source	$D_{\rm opt}$	$\Delta v$	$\tau_{\rm opt}$	$\dot{E}_{\rm kin,obs}$	$\dot{E}_{\rm kin,ext}$	$\dot{E}_{\rm shell}$
(1)	(2)	(3)	(4)	(5)	(6)	(7)
MRC0316-257	21 $\times$ 9	670	3.1			44.4
MRC0406-244	30 $\times$ 9	960	2.9	45.3	45.6	45.0
TXS0828+193	28 $\times$ 10	800	4.1	45.3	45.3	45.0
MRC1138-262	53 $\times$ 32	800	1	44.2		45.6

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