Table 2
Morphological classification and core removal.
| Name | Separation | Subpeak(s) | Type | Core | |
| arcmin | kpc | arcmin | |||
|
|
|||||
| A0160 | 0.72 | 37.8 | Y | 2 | – |
| A1177 | 0.16 | 6.0 | Y | 2 | – |
| ESO 552020 | 0.43 | 17.4 | N | 1 | – |
| HCG 62 | 0.18 | 3.0 | N | 1 | 2.00 |
| HCG 97 | 0.27 | 7.2 | N | 1 | – |
| IC 1262 | 0.51 | 21.0 | N | 1 | 0.85 |
| IC 1633 | 1.54 | 46.1 | N | 2 | – |
| MKW4 | 0.22 | 5.3 | N | 1 | 0.68 |
| MKW8 | 1.27 | 41.3 | N | 2 | – |
| NGC 326 | 1.19 | 65.8 | N | 2 | – |
| NGC 507 | 0.08 | 1.9 | N | 1 | 1.41 |
| NGC 533 | 0.23 | 4.9 | N | 1 | 1.02 |
| NGC 777 | 0.40 | 8.2 | N | 1 | – |
| NGC 1132 | 0.27 | 7.8 | N | 1 | – |
| NGC 1550 | 0.22 | 3.3 | N | 1 | 0.59 |
| NGC 4325 | 0.04 | 1.3 | N | 1 | 0.67 |
| NGC 4936 | 0.57 | 8.3 | N | 1 | – |
| NGC 5129 | 0.16 | 4.4 | N | 1 | – |
| NGC 5419 | 0.76 | 13.0 | N | 1 | – |
| NGC 6269 | 0.22 | 9.0 | N | 1 | 1.62 |
| NGC 6338 | 0.42 | 14.3 | Y | 2 | 1.92 |
| NGC 6482 | 0.07 | 1.1 | N | 1 | – |
| RXC J1022.0+3830 | 0.11 | 6.2 | N | 1 | – |
| RXC J2214.8+1350 | 0.45 | 14.3 | N | 1 | – |
| S0463 | 3.24 | 151.7 | Y | 2 | – |
| SS2B153 | 0.08 | 1.5 | N | 1 | – |
Notes. An object is classified as morphology type 2 (disturbed) if the separation between emission peak and emission-weighted center is >30 kpc and/or if there are several distinct peaks visible in the X-ray emission. The last column is the low-temperature core excised when fitting the global temperature (see Sect. 3.1).
Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.
Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.
Initial download of the metrics may take a while.