Metallicity Maps: X‐ray Observation Versus Simulation

In our simulated and observed metal maps of galaxy cluster we see a very inhomogeneous distribution, it shows stripes and blobs. We want to quantify these inhomogeneities with statistical measures in order to compare observed and simulated metal maps. Since the metal maps are the ideal diagnostic tools to study the enrichment processes, our goal is to study the efficiency of the various enrichment processes in different cluster environments.