Table 1.
Systems with X-ray flux greater than 9 × 10−12 erg cm−2 s−1 from the sample of Ebeling et al. (1998), and with an Hα luminosity greater than 1040 erg s−1 from the sample of Crawford et al. (1999), ordered by decreasing Hα luminosity.
| Object | fX | LHα | Literature |
|---|---|---|---|
| [erg cm−2 s−1] | [erg s−1] | (e.g.) | |
| Abell 1068 | 9.4 × 10−12 | 172.3 × 1040 | (1), (2) |
| Abell 1835 | 14.7 × 10−12 | 163.9 × 1040 | (3), (4) |
| Abell 2204 | 21.9 × 10−12 | 159.4 × 1040 | (5), (6) |
| Abell 2390 | 9.6 × 10−12 | 61.6 × 1040 | (7), (8) |
| RXJ1720+26 | 14.3 × 10−12 | 12.7 × 1040 | (9) |
| Abell 115 | 9.0 × 10−12 | 12.7 × 1040 | (10) |
| ZwCl 8276 | 16.4 × 10−12 | 12.5 × 1040 | (11) |
| Abell 1795 | 68.1 × 10−12 | 11.3 × 1040 | (12), (13) |
| Abell 478 | 39.9 × 10−12 | 10.8 × 1040 | (14) |
| 2A0335+096 | 80.5 × 10−12 | 10.3 × 1040 | (15), (16) |
| Abell 2009 | 9.2 × 10−12 | 6.1 × 1040 | (...) |
| ZwCl 235 | 10.9 × 10−12 | 4.1 × 1040 | (...) |
| Abell 2199 | 96.8 × 10−12 | 2.7 × 1040 | (17) |
| Abell 2052 | 47.1 × 10−12 | 2.6 × 1040 | (18), (19) |
| Abell 1668 | 9.3 × 10−12 | 2.3 × 1040 | (20) |
| Abell 2495 | 11.8 × 10−12 | 2.0 × 1040 | (21) |
| Abell 2634 | 23.1 × 10−12 | 1.3 × 1040 | (22), (23) |
| Abell 1991 | 9.4 × 10−12 | 1.1 × 1040 | (24), (25) |
Notes. The target of our study (ZwCl 235) is highlighted in red. (1) Object name; (2) X-ray flux; (3) Hα luminosity; (4) Examples of relevant literature studies dedicated to the object: (1) McNamara et al. (2004); (2) Wise et al. (2004); (3) McNamara et al. (2006); (4) McNamara et al. (2014); (5) Sanders et al. (2009a); (6) Chen et al. (2017); (7) Allen et al. (2001); (8) Sonkamble et al. (2015); (9) Mazzotta et al. (2001); (10) Hallman et al. (2018); (11) Ettori et al. (2013); (12) Kokotanekov et al. (2018); (13) Russell et al. (2017); (14) Sun et al. (2003); (15) Sanders et al. (2009b); (16) Vantyghem et al. (2016); (17) Nulsen et al. (2013); (18) Blanton et al. (2011); (19) Balmaverde et al. (2018); (20) Pasini et al. (2021); (21) Pasini et al. (2019); (22) Schindler & Prieto (1997); (23) Sun et al. (2007); (24) Sharma et al. (2004); and (25) Hamer et al. (2012).
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