Heating the bubbly gas of galaxy clusters with weak shocks and sound waves

S. Heinz; E. Churazov

doi:10.1086/498301

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Heating the bubbly gas of galaxy clusters with weak shocks and sound waves

S. Heinz·E. Churazov

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Abstract

Using hydrodynamic simulations and a technique to extract the rotational component of the velocity field, we show how bubbles of relativistic gas inflated by AGN jets in galaxy clusters act as a catalyst, transforming the energy carried by sound and shock waves to heat. The energy is stored in a vortex field around the bubbles which can subsequently be dissipated. The efficiency of this process is set mainly by the fraction of the cluster volume filled by (sub-)kpc scale filaments and bubbles of relativistic plasma.

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S. Heinz, E. Churazov. 2005-09-26. Heating the bubbly gas of galaxy clusters with weak shocks and sound waves. https://doi.org/10.1086/498301

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