An idealized simulation of a relaxed Perseus-like cluster shows that combined jet-wind AGN feedback, with GRMHD-constrained properties, reproduces key observables by boosting heating efficiency through shear-driven turbulence.
AGN Feedback in Elliptical Galaxies: Numerical Simulations
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Solving the cooling flow problem with combined jet-wind AGN feedback
An idealized simulation of a relaxed Perseus-like cluster shows that combined jet-wind AGN feedback, with GRMHD-constrained properties, reproduces key observables by boosting heating efficiency through shear-driven turbulence.