3D Metallicity and Temperature Distribution
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Metallicity distribution (blue-green) and temperature distrbution (red colormap) in a (10 Mpc)^3 cube. The stripped material from galaxies within the cluster and the Interaction with shockfronts going outwards due to a merger process can be seen. The simulation starts at z=1 and extends to roughly 10 Gyrs into the future.
 
Institute for Astrophysics, University of Innsbruck