Properties of the intracluster medium in galaxy clusters from cosmological hydrodynamical simulations
by
Veronica Biffi(University of Trieste & INAF-OATs)
→
Europe/Rome
Aula 4 (Dipartimento di Fisica - Ed. E.Fermi)
Aula 4
Dipartimento di Fisica - Ed. E.Fermi
Description
Investigating cluster properties is crucial to validate our understanding of
the main physical processes driving the formation and evolution of cosmic
structures.
Cosmological hydrodynamical simulations, able to successfully reproduce many
of the observed properties of galaxy clusters, allow us to study their
intrinsic structure and evolution, and interpret the great amount of data
expected from up-coming observational missions (e.g. Athena, eRosita, etc.).
I will present results on the thermo-dynamical and chemical properties of a
sample of galaxy clusters from simulations with AGN feedback.
