Table 4.
Properties of the cavities in our sample derived using the traditional X-ray method.
| (a) | (b) | (c) | (d) | (e) | (f) | (g) | (h) | (i) |
|---|---|---|---|---|---|---|---|---|
| Cluster name | p | Rl | Rw | R | V | tbuoy | Pcav | Ref. |
| (keV/cm3) | (kpc) | (kpc) | (kpc) | (kpc3) | (107 yr) | (1042 erg/s) | ||
| Perseus (N) | 0.4478 | 8.2 | 4.7 | 6.5 |  |
 |
 |
(1) |
| Perseus (S) | 0.387 | 9.1 | 7.3 | 9.4 |  |
 |
 |
(1) |
| Abell 2199 (E) | 0.1251 | 15 | 10 | 19 |  |
 |
 |
(1) |
| Abell 2199 (W) | 0.1205 | 16 | 10 | 21 |  |
 |
 |
(1) |
| 2A 0335+096 | 0.1291 | 9.3 | 6.5 | 23 |  |
 |
 |
(1) |
| 2A 0335+096 | 0.1125 | 4.8 | 2.6 | 28 |  |
 |
0.98 ± 0.12 | (1) |
| MKW 3S | 0.0675 | 54 | 23 | 59 |  |
 |
 |
(1) |
| Abell 1795 | 0.242 | 19 | 7.2 | 19 |  |
 |
 |
(1) |
| Abell 1668 (N) | 0.0836 | 2.6 | 1.5 | 3.5 |  |
 |
 |
(2) |
| Abell 1668 (NW) | 0.0836 | 2.4 | 2.4 | 3.5 |  |
 |
 |
(2) |
| Abell 2029 | 0.3612 | 13 | 7.2 | 32 |  |
 |
 |
(1) |
| 3C 388 (E) | 0.0436 | 15 | 15 | 27 |  |
 |
 |
(1) |
| 3C 388 (W) | 0.0486 | 24 | 10 | 21 |  |
 |
 |
(1) |
| ZwCl 2701 (E) | 0.7802 | 12.25 | 8.75 | 18.9 |  |
 |
 |
(3) |
| ZwCl 2701 (W) | 0.8364 | 14.0 | 10.5 | 19.25 |  |
 |
 |
(3) |
| MS 0735.6+7421 (N) | 0.0469 | 110 | 87 | 160 |  |
 |
 |
(1) |
| MS 0735.6+7421 (S) | 0.409 | 130 | 89 | 180 |  |
 |
 |
(1) |
| 4C+55.16 (NW) | 0.3135 | 13 | 9.4 | 22 |  |
 |
 |
(1) |
| 4C+55.16 (S) | 0.4338 | 10 | 7.5 | 16 |  |
 |
 |
(1) |
Notes. (a) cluster name; (b) ICM pressure; (c) cavity radius along the jet axis; (d) cavity radius perpendicular to the jet axis; (e) cavity distance from the AGN core; (f) cavity volume; (g) buoyancy timescale; (h) cavity power; (i) reference.
References. (1) Rafferty et al. (2006); (2) Pasini et al. (2021); (3) Vagshette et al. (2016).
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