How quickly does the gas that is heated by the SSC cool? The larger the cluster the more radiative cooling (I did not understand why) and eventually there is a regime of “catastrophic cooling” where no equilibrium solution exists any more.
Studies in M82 which blows a huge bipolar wind perpendicular to the disk (pretty picture) show that …. I missed it because I fetched the link to the picture. 
Tags: IAU2006
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