In simulations of a Perseus-like cluster with observed-level pre-existing turbulence, turbulent heating is insufficient to balance cooling in the core, and the XRISM central velocity rise is transient jet-driven bulk flow.
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Simulating AGN feedback in galaxy clusters with pre-existing turbulence
In simulations of a Perseus-like cluster with observed-level pre-existing turbulence, turbulent heating is insufficient to balance cooling in the core, and the XRISM central velocity rise is transient jet-driven bulk flow.