Physics
Scientific paper
Sep 2005
adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2005cxo..prop.2031j&link_type=abstract
Chandra Proposal ID #07800655
Physics
Chandra Proposal Id #07800655
Scientific paper
We propose to observe two galaxy clusters that contain powerful central radio sources. The sources are powerful not only in absolute terms, but in relative terms (radio to X-ray flux ratios) they are amongst the most extreme objects; more so even than well-known clusters such as Hydra~A. Our aim is to investigate the influence of radio sources on the central cluster regions, and in particular their role in disrupting cooling flows. By examining the upper boundary of the relative radio energy input distribution, we aim to shed light on the processes at work in more typical objects.
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