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Table 1.
Properties of the hot and cool components in the centers of Perseus cluster, Centaurus cluster, and Abell 1795, within the specified radius.
Objects | Perseus (a) | Centaurus (b) | Abell 1795 (c) |
---|---|---|---|
Radius (kpc) | 60 | 150 | 144 |
Cool kT (keV) | 2.9−3.6 | 1.7−2.0 | 2.0−2.5 |
Hot kT (keV) | 4.5−4.7 | 3.8 | 4.7−6.3 |
Cool LX(d) | 4.1 | 0.1 | 1.4 |
Hot LX(d) | 2.2 | 0.3 | 2.5 |
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