Non-steady heating of cool cores of galaxy clusters by ubiquitous turbulence and AGN
Yutaka Fujita, Renyue Cen, Irina Zhuravleva

TL;DR
This study uses hydrodynamic simulations to explore how turbulence and AGN feedback stabilize cool cores in galaxy clusters, revealing intermittent AGN activity and a self-regulating heating-cooling balance.
Contribution
It demonstrates that turbulence and AGN feedback together maintain core stability, with intermittent AGN activity and rapid heating events, advancing understanding of cluster core dynamics.
Findings
AGN activity is intermittent with turbulence similar to Hitomi observations.
Core maintains quasi-equilibrium due to turbulent diffusion balancing cooling.
AGN bursts heat the core rapidly without causing global instability.
Abstract
Recent cosmological simulations have shown that turbulence should be generally prevailing in clusters because clusters are continuously growing through matter accretion. Using one-dimensional hydrodynamic simulations, we study the heating of cool-core clusters by the ubiquitous turbulence as well as feedback from the central active galactic nuclei (AGNs) for a wide range of cluster and turbulence parameters, focusing on the global stability of the core. We find that the AGN shows intermittent activities in the presence of moderate turbulence similar to the one observed with Hitomi. The cluster core maintains a quasi-equilibrium state for most of the time because the heating through turbulent diffusion is nearly balanced with radiative cooling. The balance is gradually lost because of slight dominance of the radiative cooling, and the AGN is ignited by increased gas inflow. Finally, when…
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