Rhapsody-C simulations -- Anisotropic thermal conduction, black hole physics, and the robustness of massive galaxy cluster scaling relations

Alisson Pellissier, Oliver Hahn, Chiara Ferrari

We present the Rhapsody-C simulations that extend the Rhapsody-G suite of massive galaxy clusters at the $M_{\mathrm{vir}}\sim 10^{15}{\mathrm{M}}_{\odot }$ scale with cosmological m…