Physical properties of very powerful FRII radio galaxies

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Table 4:

Summary of source properties. II.
Source	T_{T (b=0.25)}	E_{T (b=0.25)}	T_{T (b=1)}	E_{T (b=1)}
	10⁷ yr	10⁶ $M_{\odot}$	10⁷ yr	10⁶ $M_{\odot}$
3C 239	$1.2 \pm 0.4$	$5.1 \pm 1.5$	$0.17 \pm 0.04$	$1.02 \pm 0.26$
3C 322	$1.2 \pm 0.3$	$5.2 \pm 1.5$	$0.18 \pm 0.05$	$0.97 \pm 0.25$
3C 322	$1.2 \pm 0.4$	$5.4 \pm 1.7$	$0.16 \pm 0.05$	$1.04 \pm 0.31$
3C 68.2	$2.1 \pm 0.7$	$3.0 \pm 1.0$	$0.29 \pm 0.09$	$0.59 \pm 0.19$
3C 68.2	$1.6 \pm 0.5$	$4.0 \pm 1.2$	$0.21 \pm 0.06$	$0.81 \pm 0.22$
3C 437	$1.1 \pm 0.3$	$5.7 \pm 1.6$	$0.16 \pm 0.04$	$1.05 \pm 0.26$
3C 437	$0.7 \pm 0.2$	$9.1 \pm 2.6$	$0.09 \pm 0.02$	$1.83 \pm 0.46$
3C 324	$2.2 \pm 0.7$	$2.9 \pm 1.0$	$0.29 \pm 0.09$	$0.59 \pm 0.18$
3C 194	$3.9 \pm 1.3$	$1.6 \pm 0.5$	$0.55 \pm 0.16$	$0.31 \pm 0.09$
3C 194	$3.2 \pm 1.0$	$1.9 \pm 0.6$	$0.45 \pm 0.12$	$0.38 \pm 0.10$
3C 267	$1.9 \pm 0.6$	$3.3 \pm 1.0$	$0.26 \pm 0.07$	$0.65 \pm 0.18$
3C 267	$1.9 \pm 0.6$	$3.2 \pm 0.9$	$0.27 \pm 0.07$	$0.63 \pm 0.17$
3C 356	$1.8 \pm 0.6$	$3.4 \pm 1.1$	$0.28 \pm 0.08$	$0.62 \pm 0.18$
3C 356	$1.4 \pm 0.4$	$4.6 \pm 1.5$	$0.19 \pm 0.06$	$0.88 \pm 0.25$
3C 280	$2.3 \pm 0.7$	$2.7 \pm 0.8$	$0.31 \pm 0.08$	$0.54 \pm 0.14$
3C 280	$4.0 \pm 1.2$	$1.6 \pm 0.4$	$0.58 \pm 0.15$	$0.29 \pm 0.08$
3C 268.1	$2.7 \pm 0.8$	$2.3 \pm 0.7$	$0.40 \pm 0.11$	$0.43 \pm 0.11$
3C 268.1	$1.8 \pm 0.5$	$3.5 \pm 1.0$	$0.25 \pm 0.06$	$0.69 \pm 0.18$
3C 289	$3.1 \pm 0.9$	$2.0 \pm 0.6$	$0.42 \pm 0.11$	$0.41 \pm 0.10$
3C 289	$2.7 \pm 0.8$	$2.3 \pm 0.7$	$0.36 \pm 0.09$	$0.47 \pm 0.12$
3C 325	$5.1 \pm 2.0$	$1.2 \pm 0.5$	$0.72 \pm 0.24$	$0.24 \pm 0.08$
3C 325	$1.6 \pm 0.5$	$4.0 \pm 1.3$	$0.21 \pm 0.06$	$0.82 \pm 0.24$
3C 265	$2.7 \pm 0.8$	$2.3 \pm 0.7$	$0.37 \pm 0.10$	$0.46 \pm 0.12$
3C 265	$4.1 \pm 1.3$	$1.5 \pm 0.5$	$0.62 \pm 0.17$	$0.27 \pm 0.08$
3C 247	$3.4 \pm 1.0$	$1.8 \pm 0.5$	$0.47 \pm 0.13$	$0.36 \pm 0.10$
3C 247	$4.8 \pm 1.4$	$1.3 \pm 0.4$	$0.65 \pm 0.17$	$0.26 \pm 0.07$
3C 55	$1.9 \pm 0.6$	$3.2 \pm 0.9$	$0.27 \pm 0.07$	$0.64 \pm 0.17$
3C 55	$2.1 \pm 0.6$	$3.0 \pm 0.9$	$0.29 \pm 0.08$	$0.60 \pm 0.17$
3C 337	$6.6 \pm 2.1$	$0.9 \pm 0.3$	$1.05 \pm 0.30$	$0.16 \pm 0.05$
3C 337	$4.0 \pm 1.1$	$1.6 \pm 0.4$	$0.61 \pm 0.15$	$0.28 \pm 0.07$
3C 427.1	$4.5 \pm 1.3$	$1.4 \pm 0.4$	$0.62 \pm 0.16$	$0.28 \pm 0.07$
3C 427.1	$5.0 \pm 1.4$	$1.2 \pm 0.4$	$0.68 \pm 0.18$	$0.25 \pm 0.07$
3C 330	$2.8 \pm 0.8$	$2.3 \pm 0.7$	$0.38 \pm 0.10$	$0.45 \pm 0.12$
3C 330	$3.1 \pm 0.9$	$2.0 \pm 0.6$	$0.44 \pm 0.12$	$0.39 \pm 0.10$
3C 244.1	$8.3 \pm 2.3$	$0.8 \pm 0.2$	$1.24 \pm 0.31$	$0.14 \pm 0.03$
3C 244.1	$5.0 \pm 1.4$	$1.2 \pm 0.3$	$0.70 \pm 0.17$	$0.24 \pm 0.06$
3C 405	$3.7 \pm 1.0$	$1.7 \pm 0.4$	$0.48 \pm 0.12$	$0.36 \pm 0.09$
3C 405	$4.1 \pm 1.1$	$1.5 \pm 0.4$	$0.52 \pm 0.13$	$0.33 \pm 0.08$
3C 6.1	$3.1 \pm 0.8$	$2.0 \pm 0.5$	$0.50 \pm 0.12$	$0.34 \pm 0.08$
3C 6.1	$2.4 \pm 0.6$	$2.7 \pm 0.7$	$0.42 \pm 0.10$	$0.40 \pm 0.10$
3C 34	$2.4 \pm 0.6$	$2.6 \pm 0.7$	$0.46 \pm 0.11$	$0.37 \pm 0.09$
3C 34	$3.6 \pm 0.9$	$1.7 \pm 0.4$	$0.71 \pm 0.16$	$0.24 \pm 0.06$
3C 41	$4.6 \pm 1.2$	$1.4 \pm 0.4$	$0.91 \pm 0.22$	$0.19 \pm 0.05$
3C 41	$3.0 \pm 0.7$	$2.1 \pm 0.5$	$0.49 \pm 0.12$	$0.35 \pm 0.08$
3C 44	$3.6 \pm 0.9$	$1.7 \pm 0.4$	$0.58 \pm 0.14$	$0.29 \pm 0.07$
3C 44	$3.6 \pm 0.9$	$1.8 \pm 0.4$	$0.58 \pm 0.14$	$0.29 \pm 0.07$
3C 54	$2.3 \pm 0.6$	$2.8 \pm 0.7$	$0.45 \pm 0.11$	$0.38 \pm 0.09$
3C 54	$2.7 \pm 0.7$	$2.3 \pm 0.6$	$0.44 \pm 0.10$	$0.38 \pm 0.09$
3C 114	$2.2 \pm 0.6$	$2.8 \pm 0.7$	$0.47 \pm 0.11$	$0.36 \pm 0.08$
3C 114	$2.3 \pm 0.6$	$2.8 \pm 0.7$	$0.48 \pm 0.11$	$0.35 \pm 0.08$
3C 142.1	$5.2 \pm 1.2$	$1.2 \pm 0.3$	$0.76 \pm 0.18$	$0.23 \pm 0.05$
3C 142.1	$3.6 \pm 0.9$	$1.7 \pm 0.4$	$0.62 \pm 0.15$	$0.28 \pm 0.07$
3C 169.1	$3.3 \pm 0.9$	$1.9 \pm 0.5$	$0.75 \pm 0.18$	$0.23 \pm 0.05$
3C 169.1	$3.3 \pm 0.8$	$1.9 \pm 0.5$	$0.64 \pm 0.15$	$0.27 \pm 0.06$
3C 172	$4.9 \pm 1.3$	$1.3 \pm 0.3$	$0.85 \pm 0.21$	$0.20 \pm 0.05$
3C 172	$1.5 \pm 0.5$	$4.2 \pm 1.5$	$0.28 \pm 0.09$	$0.62 \pm 0.21$
3C 441	$3.6 \pm 0.9$	$1.8 \pm 0.4$	$0.71 \pm 0.17$	$0.24 \pm 0.06$
3C 441	$2.0 \pm 0.5$	$3.1 \pm 0.8$	$0.35 \pm 0.09$	$0.49 \pm 0.12$
3C 469.1	$1.0 \pm 0.3$	$6.3 \pm 1.6$	$0.17 \pm 0.04$	$0.97 \pm 0.24$
3C 469.1	$0.9 \pm 0.2$	$7.2 \pm 1.8$	$0.16 \pm 0.04$	$1.04 \pm 0.25$

The top part of the table contains the properties of the previous sample of 20 radio sources recalculated for the currently adopted cosmology. The bottom part of the table contains the new sample of 11 radio galaxies. Column 1: source name, Col. 2: the total lifetime of the outflow (b=0.25), Col. 3: the total energy of the outflow (b=0.25), Col. 4: the total lifetime of the outflow (b = 1), Col. 5: the total energy of the outflow (b = 1).

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