F
C
Last name: FERRARI
First name: Chiara
International audience
In the framework of the hierarchical model of structure formation,galaxy clusters are supposed to form by accretion and merging ofsmaller units.I present our multi-wavelength (optical, X-ray and radio) observation program of a sample of morphologically complex clusters, representing the different phases of the merging process ("MUSIC:...
International audience
We present the Rhapsody-C simulations that extend the Rhapsody-G suite of massive galaxy clusters at the $M_{\rm vir}\sim10^{15}\thinspace{\rm M}_{\odot}$ scale with cosmological magneto-hydrodynamic zoom-in simulations that include anisotropic thermal conduction, modified supermassive black hole (SMBH) feedback, new SMBH seeding and SMBH...