期刊
ASTROPHYSICAL JOURNAL
卷 634, 期 2, 页码 L141-L144出版社
IOP PUBLISHING LTD
DOI: 10.1086/498301
关键词
galaxies : clusters : general; hydrodynamics; instabilities; ISM : bubbles methods : numerical; shock waves
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 into 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-) kiloparsec-scale filaments and bubbles of relativistic plasma.
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