Nustar view of the central region of the Perseus cluster
B. Rani, G. M. Madejski, R. F. Mushotzky, C. Reynolds, J. A. Hodgson

TL;DR
This study presents NuSTAR observations of the central AGN in the Perseus cluster, revealing a dominant hard X-ray power-law component likely originating from the jet, with spectral analysis ruling out thermal accretion disk emission.
Contribution
First NuSTAR spectral analysis of 3C 84 that decomposes the AGN's hard X-ray emission and suggests a jet origin over thermal accretion disk processes.
Findings
Power-law component dominates above 20 keV with photon index ~1.9
Hard X-ray flux correlates with hardness ratio variations
Thermal emission from the accretion disk is insufficient to explain observed X-rays
Abstract
Located at the center of the Perseus cluster, 3C 84 is an extremely bright and nearby radio galaxy. Because of the strong diffuse thermal emission from the cluster in X-rays, the detailed properties and the origin of a power-law component from the central active galactic nucleus (AGN) remains unclear in the source. We report here the first NuSTAR observations of 3C 84. The source was observed for 24.2 and 32 ks on February 01 and 04, 2018, respectively. NuSTAR observations spectrally decompose the power-law AGN component above 10 keV. The power-law component dominates the spectrum above 20 keV with a photon index 1.9 and an energy flux F = 1.0 10 erg cm s, corresponding to an isotropic luminosity, = 7.410 erg s. We discuss possible emitting sites for the power-law component. The expected thermal…
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