Table 2.
Parameters of the cluster models with a rotating ICM.
| Model | Halo | Rbreak [kpc] | n⋆ [cm−3] | T⋆ [keV] | u0 [km s−1] | R0 [kpc] |
 |
 |
|---|---|---|---|---|---|---|---|---|
| SRM | SDM | 380 | 2.5 × 10−3 | 7.3 | 1900 | 280 | 0.83 | 1.19 |
| ORM | ODM | 420 | 2.2 × 10−3 | 7.4 | 1800 | 180 | 0.82 | 1.20 |
| PRM | PDM | 360 | 2.5 × 10−3 | 7.4 | 2300 | 280 | 0.84 | 1.19 |
Notes. We refer to these cluster models with a rotating ICM as the “spherical rotating model” (SRM), the “oblate rotating model” (ORM), and the “prolate rotating model” (PRM), depending on the spherical, oblate, and prolate DM halo models assumed, respectively. The corresponding SDM, PDM, and ODM halo models (cited in the second column) are defined in Sect. 2.2.
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