Heating the intra-cluster medium perpendicular to the jets axis
Avishai Gilkis, Noam Soker (Technion, Israel)

TL;DR
Simulations show that mixing of shocked jet material with the intra-cluster medium efficiently heats the gas perpendicular to the jets' axis, sustaining heating long after jet activity ceases and impacting magnetic fields and galaxy evolution.
Contribution
This study demonstrates that mixing, rather than shock heating, is the dominant process heating the intra-cluster medium perpendicular to jets in galaxy clusters.
Findings
Mixing heats the ICM efficiently up to ~10 kpc and beyond.
Heating persists for over 10^8 years after jet activity ends.
Mixing influences magnetic fields and supports cold feedback mechanisms.
Abstract
By simulating jet-inflated bubbles in cooling flows with the PLUTO hydrodynamic code we show that mixing of high entropy shocked jet's material with the intra-cluster medium (ICM) is the major heating process perpendicular to the jets' axis. Heating by the forward shock is not significant. The mixing is very efficient in heating the ICM in all directions, to distances of ~10kpc and more. Although the jets are active for a time period of only 20 Myr, the mixing and heating near the equatorial plane, as well as along the symmetry axis, continues to counter radiative cooling for times of >10^8 yr after the jets have ceased to exist. We discuss some possible implications of the results. (i) The vigorous mixing is expected to entangle magnetic field lines, hence to suppress any global heat conduction in the ICM near the center. (ii) The vigorous mixing forms multi-phase ICM in the inner…
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