Table 5
Cluster properties.
Cluster name | Source name | n0 | rc | β | r | n r | Notes | Ref. | |
10-3 cm-3 | kpc | kpc | 10-3 cm-3 | ||||||
|
|||||||||
A 278 | J0157+3214 | 1.8 | 175 | 0.70 | 217 | 0.68 | merging | 1 | |
A 520 | J0454+0255A | 3.8 | 413 | 0.87 | 269 | 2.4 | merging | 2 | |
J0454+0255B | 358 | 1.8 | |||||||
A 869 | J0946+0222 | no data | |||||||
A 1775 | J1341+2622 | 3.3 | 122 | 0.58 | 58.5 | 2.7 | merging | 3 | |
A 1795 | J1348+2633 | 36 | 242 | 0.79 | 181 | 17 | cool core | 4 | |
A 2142 | J1558+2716 | 19 | 447 | 0.79 | 292 | 13 | merging/cool core | 4 | |
A 2255 | J1713+6407 | 2.1 | 411 | 0.79 | 350 | 1.1 | merging | 4 | |
A 2256 | J1703+7839 | 3.6 | 342 | 0.83 | 211 | 2.5 | merging | 4 | |
J1700+7841 | 596 | 0.65 | |||||||
Ophiuchus | J1712–2328 | 19 | 187 | 0.70 | 212 | 8.2 | cool core | 4 |
Notes. Column 1: cluster name; Col. 2: source name; Cols. 3–5: parameters of the cluster gas density distribution according to Eq. (2); Col. 6: projected distance of the radio galaxy from the cluster center; Col. 7: gas density at the radio galaxy location; Col. 8: note on the cluster dynamical status; Col. 9: reference to the cluster gas data (here scaled to the adopted cosmology), 1 = Feretti et al. (1990); 2 = Govoni et al. (2001); 3 = Cirimele et al. (1997); and 4 = Mohr et al. (1999).
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