Metallicity Maps: X-ray Observation Versus Simulation

Details Metallicity Maps: X-ray Observation Versus Simulation Metallicity Maps: X-ray Observation Versus Simulation

May 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1126..290l&link_type=abstract

SIMBOL-X: FOCUSING ON THE HARD X-RAY UNIVERSE: Proceedings of the 2nd International Simbol-X Symposium. AIP Conference Proceedi

Computer Science

1

Galaxy Groups, Clusters, And Superclusters, Large Scale Structure Of The Universe, Galactic Nuclei, Circumnuclear Matter, And Bulges, X-Ray

Scientific paper

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.

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