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Table 2.
Cosmic X-ray background information for the spectral analysis of the Centaurus cluster.
Component | Parameter | Value |
---|---|---|
apec1 (LHB) | kBT(456) [keV] | ![]() |
Z [Z⊙] | 1 | |
z | 0 | |
norm( * ,456) | ![]() |
|
apec2 (MWH) | kBT(456) [keV] | ![]() |
Z [Z⊙] | 1 | |
z | 0 | |
norm( * ,456) | (1.71 ± 0.05)×10−6 | |
apec3 | kBT(1) [keV] | ![]() |
(eROSITA Bubbles) | Z [Z⊙] | 1 |
z | 0 | |
norm( * ,456) | < 2.80 × 10−8 | |
powerlaw | Γ | 1.46 |
(unresolved sources) | norm( ‡ ,456) | ![]() |
Notes. (456)from combined box 4N, 5N, 6N, 4S, 5S, and 6S, (1) from combined box 1N and 1S. ( † )[1022 atoms cm−2], ( * )[cm−5/arcmin2], ( ‡ )[photons/keV/cm2/s/arcmin2 at 1 keV].
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