Table 5.
Properties of the cavities in our sample derived using the hybrid X-ray–radio method.
| (a) | (b) | (c) | (d) | (e) | (f) | (g) | (h) |
|---|---|---|---|---|---|---|---|
| Cluster name | Rl | Rw | R | V | tbuoy | Pcav | Ref. |
| (kpc) | (kpc) | (kpc) | (kpc3) | (107 yr) | (1042 erg/s) | ||
| Perseus (N) | 6.7 | 5.9 | 6.6 |
 |
 |
 |
(1) |
| Perseus (S) | 4.3 | 3.4 | 4.5 |
 |
 |
 |
(1) |
| Abell 1795 (N) | 2.2 | 2.3 | 3.5 |
 |
 |
 |
(1) |
| Abell 1795 (S) | 5.5 | 2.3 | 4.7 |
 |
 |
 |
(1) |
| Abell 2029 (N) | 9.0 | 3.9 | 10.8 |
 |
 |
 |
(1) |
| 9.2 | 5.0 | 31.6 |
 |
 |
 |
(1) | |
| Abell 2029 (S) | 6.1 | 2.7 | 8.2 |
 |
 |
 |
(1) |
| 19.5 | 3.9 | 27.1 |
 |
 |
 |
(1) | |
| ZwCl 2701 (E) | 8.4 | 5.6 | 22.3 |
 |
 |
 |
(1) |
| ZwCl 2701 (W) | 12.7 | 6.3 | 23.3 |
 |
 |
 |
(1) |
| 4C+55.16 (NW) | 12.6 | 7.4 | 16.0 |
 |
 |
 |
(1) |
| 4C+55.16 (S) | 13.5 | 6.7 | 20.9 |
 |
 |
 |
(1) |
| Perseus (N) | 7.2 | 8.6 | 6.9 |
 |
 |
 |
(1) |
| Perseus (S) | 4.4 | 4.1 | 4.3 |
 |
 |
 |
(1) |
| Abell 2199 (E) | 12.8 | 6.0 | 16.2 |
 |
 |
 |
(2) |
| Abell 2199 (W) | 14.1 | 7.8 | 19.2 |
 |
 |
 |
(2) |
| 2A 0335+096 (NW) | 10.2 | 9.4 | 27.0 |
 |
 |
 |
(3) |
| 2A 0335+096 (SE) | 5.5 | 7.8 | 22.9 |
 |
 |
 |
(3) |
| MKW 3S | 25.4 | 46.4 | 50.0 |
 |
 |
 |
(2) |
| Abell 1668 (NE) | 13.0 | 7.4 | 31.0 |
 |
 |
 |
(2) |
| Abell 1668 (S) | 9.9 | 9.3 | 34.0 |
 |
 |
 |
(2) |
| Abell 2029 (N) | 21.8 | 4.3 | 21.4 |
 |
 |
 |
(2) |
| Abell 2029 (S) | 26.0 | 4.7 | 22.3 |
 |
 |
 |
(2) |
| 3C 388 (E) | 17.3 | 13.7 | 23.3 |
 |
 |
 |
(2) |
| 3C 388 (W) | 12.8 | 20.7 | 21.6 |
 |
 |
 |
(2) |
| MS 0735.6+7421 (N) | 111 | 112 | 138 |
 |
 |
 |
(4) |
| MS 0735.6+7421 (S) | 128 | 115 | 173 |
 |
 |
 |
(4) |
Notes. The horizontal line separates the clusters that are studied at high resolutions (top half) from the clusters that are studied at low resolutions (bottom half). (a) cluster name; (b) cavity radius along the jet axis; (c) cavity radius perpendicular to the jet axis; (d) cavity distance from the AGN core; (e) cavity volume; (f) buoyancy timescale; (g) cavity power; (h) reference for radio observations.
References. (1) This paper; (2) LoTSS; (3) Ignesti et al. (2022); (4) Biava et al. (2021).
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