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Source | z | r | (v/c) | (v/c) | aL | P10 | Lj | na |
kpc | (b=0.25) | (b=1) | kpc | 10-10 dynes cm-2 | 1044erg s-1 | 10-3 cm-3 | ||
3C 239 | 1.790 | 69.5 |
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3C 322 | 1.681 | 139.4 |
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3C 322 | 1.681 | 185.3 |
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3C 68.2 | 1.575 | 104.7 |
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3C 68.2 | 1.575 | 115.8 |
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3C 437 | 1.480 | 168.4 |
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3C 437 | 1.480 | 160.5 |
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3C 324 | 1.210 | 35.2 |
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3C 194 | 1.190 | 50.3 |
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3C 194 | 1.190 | 79.6 |
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3C 267 | 1.144 | 175.1 |
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3C 267 | 1.144 | 165.6 |
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3C 356 | 1.079 | 377.1 |
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3C 356 | 1.079 | 251.4 |
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3C 280 | 0.996 | 49.3 |
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3C 280 | 0.996 | 60.4 |
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3C 268.1 | 0.974 | 201.8 |
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3C 268.1 | 0.974 | 171.6 |
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3C 289 | 0.967 | 44.5 |
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3C 289 | 0.967 | 46.1 |
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3C 325 | 0.860 | 77.7 |
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3C 325 | 0.860 | 55.0 |
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3C 265 | 0.811 | 250.0 |
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3C 265 | 0.811 | 294.3 |
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3C 247 | 0.749 | 39.5 |
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3C 247 | 0.749 | 64.7 |
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3C 55 | 0.720 | 261.7 |
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3C 55 | 0.720 | 268.0 |
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3C 337 | 0.630 | 196.1 |
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3C 337 | 0.630 | 109.5 |
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3C 427.1 | 0.572 | 82.8 |
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3C 427.1 | 0.572 | 75.0 |
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3C 330 | 0.549 | 205.9 |
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3C 330 | 0.549 | 199.7 |
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3C 244.1 | 0.430 | 155.9 |
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3C 244.1 | 0.430 | 141.4 |
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3C 405 | 0.056 | 63.8 |
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3C 405 | 0.056 | 72.5 |
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3C 6.1 | 0.840 | 106.0 |
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3C 6.1 | 0.840 | 92.2 |
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3C 34 | 0.690 | 170.4 |
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3C 34 | 0.690 | 149.9 |
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3C 41 | 0.794 | 93.8 |
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3C 41 | 0.794 | 84.8 |
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3C 44 | 0.660 | 280.0 |
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3C 44 | 0.660 | 172.2 |
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3C 54 | 0.827 | 201.9 |
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3C 54 | 0.827 | 187.6 |
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3C 114 | 0.815 | 192.1 |
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3C 114 | 0.815 | 209.5 |
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3C 142.1 | 0.406 | 99.2 |
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3C 142.1 | 0.406 | 185.1 |
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3C 169.1 | 0.633 | 131.4 |
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3C 169.1 | 0.633 | 189.7 |
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3C 172 | 0.519 | 294.7 |
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3C 172 | 0.519 | 333.0 |
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3C 441 | 0.707 | 69.4 |
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3C 441 | 0.707 | 169.7 |
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3C 469.1 | 1.336 | 306.1 |
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3C 469.1 | 1.336 | 327.5 |
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All calculations follow WDW and assume b = 0.25 except where noted. 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: redshift, Col. 3: the distance between the core and hotspot, Col. 4: the source expansion speed, Col. 5: the source expansion speed for b= 1, Col. 6: the half-width of the lobe at a projected distance of 10 kpc along the ridge line from the hotspot towards the core, Col. 7: the pressure in the lobe at a projected distance of 10 kpc along the ridge line from the hotspot towards the core, Col. 8: the beam power, Col. 9: the ambient density. |
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