Cooling and clusters: when is heating needed?
There are (at least) two unsolved problems concerning the current state of the ther- mal gas in clusters of galaxies. The first is to identify the source of the heating which onsets cooling in the centres of clusters with short cooling times (the 'cooling-flow' problem). The second to understand the mechanism which boosts the entropy in cluster and group gas. Since both of these problems involve an unknown source of heating it is tempting to identify them with the same process, particularly since active galactic nuclei heating is observed to be operating at some level in a sample of well-observed 'cooling-flow' clusters. Here we show, using numerical simulations of cluster formation, that much of the gas ending up in clusters cools at high redshift and so the heating is also needed at high redshift, well before the cluster forms. This indicates that the same process operating to solve the cooling-flow problem may not also resolve the cluster-entropy problem.
Bryan
Greg
G
Department of Astrophysics, Denys Wilkinson Building, University of Oxford, Keble Road, Oxford OX1 3RH, UK. gbryan@astro.ox.ac.uk
Voit
Mark
M
D001256:Astronomy / Q000379:methods*; D005118:Extraterrestrial Environment; D006358:Hot Temperature; D008962:Models, Theoretical; D055585:Physical Phenomena; D010825:Physics; D013997:Time Factors