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Understanding the Evolution of Cool Core Clusters in Galaxies

This presentation by Joana Santos (INAF-Trieste) explores the evolution of cool core clusters, the largest gravitationally bound systems in the universe. It highlights their formation at redshifts greater than 2 and discusses the key components, including dark matter, hot gas (the intracluster medium), and galaxies. These clusters serve as exceptional cosmological probes and are ideal laboratories for studying astrophysical processes. The findings contribute to our understanding of galaxy formation and the dynamics of matter in the universe.

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Understanding the Evolution of Cool Core Clusters in Galaxies

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