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Properties of the ICM from simulations with AGN feedback
Rasia, Elena (2016)
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https://hdl.handle.net/11299/182001
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Title
Properties of the ICM from simulations with AGN feedback
Authors
Issue Date
2016-08-24
Type
Presentation
Abstract
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.
Keywords
ICM
Appears in collections
Physics of the Intracluster Medium: Theory and Computation 2016 [31]
Suggested Citation
Rasia, Elena. (2016). Properties of the ICM from simulations with AGN feedback. Retrieved from the University of Minnesota Digital Conservancy, https://hdl.handle.net/11299/182001.
Content distributed via the University of Minnesota's Digital Conservancy may be subject to additional license and use restrictions applied by the depositor.