Table 5.
X-ray derived 3D cluster model.
| Sub. | Amp. | rc [kpc] | β | RA | Dec |
|---|---|---|---|---|---|
| A | 0.577 | 785 | 1.855 | 07:17:25.0 | +37:45:54.6 |
| B | 1.483 | 279 | 0.896 | 07:17:31.3 | +37:45:30.3 |
| C | 0.851 | 166 | 0.624 | 07:17:35.8 | +37:45:01.0 |
| D | 0.977 | 145 | 0.577 | 07:17:33.0 | +37:44:15.0 |
| E | 0.549 | 69 | 0.495 | 07:17:53.3 | +37:42:11.8 |
Notes. Best-fit parameters for five spherical beta models determined from Chandra data. The central positions for sub-clusters A-D are the same shown in Table 7, and are determined form the strong lensing centres in Limousin et al. (2016), while the centre of sub-cluster E is fixed to the centre of the group region.
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