Centaurus Cluster, Chandra
Centaurus Cluster, Chandra Abell 1835, XMM-Newton

Omni Hotel, Charlottesville, VA, USA
May 31 - June 4, 2003

Recent observations have significantly broadened our view on cooling flows in galaxies and clusters of galaxies. The wealth of new information gained through observations has led to flourishing development in theoretical modelling. The purpose of this conference is to summarize relevant observational results at all wavelengths, to compare the predictions of models and simulations to these observations, and to assess the impact of processes in cluster cores on the application of galaxy clusters as cosmological probes.

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