2002/10/25 by Christian R. Kaiser, Kaiser, Christian R., Marcus Brueggen +3
Physics and Astronomy · #Astrophysics (astro-ph) #FOS: Physical sciences #astro-ph
paper · pdf · doi:10.48550/arxiv.astro-ph/0210569
Contribution to AGN2002 meeting in Paris, to appear in ASP Conference Series
arxiv created 2002/10/25 · arxiv updated 2009/12/01
We present a simple analytical model and the results of numerical simulations supporting the idea of periodical heating of cluster gas by AGN outflows. We show why, under this assumption, we are extremely unlikely to observe clusters containing gas with a temperature below about 1 keV. We review the results from numerical hydro-simulations studying the mechanisms by which AGN outflows heat the cluster gas.