Properties of the ICM from simulations with AGN feedback
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Powerful phenomena determine the energy of Galaxy Clusters from sub-pc scales to Mpc distances. Via high-resolution, cosmological and hydrodynamical simulations we studied how the main properties of the ICM (entropy, temperature, pressure, and metallicity) are influences by the presence of the central AGN. We will report on the evolution of profiles and scaling relation between global quantities including luminosity and total mass. Special focus will be given to the metallicity profile.
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Rasia, Elena. (2016). Properties of the ICM from simulations with AGN feedback. Retrieved from the University Digital Conservancy, https://hdl.handle.net/11299/182001.
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