22 citations · 69 across the 4 of their papers we have counts for
4 papers
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 scale with cosmological m…
AGN jets do not prevent the suppression of conduction by the heat buoyancy instability in simulated galaxy clusters
Ricarda S. Beckmann, Yohan Dubois, Alisson Pellissier +2
Centres of galaxy clusters must be efficiently reheated to avoid a cooling catastrophe. One potential reheating mechanism is anisotropic thermal conduction, which could transport t…
Cosmic rays and thermal instability in self-regulating cooling flows of massive galaxy clusters
Ricarda S. Beckmann, Yohan Dubois, Alisson Pellissier +5
One of the key physical processes that helps prevent strong cooling flows in galaxy clusters is the continued energy input from the central active galactic nucleus (AGN) of the clu…
The MUSE Hubble Ultra Deep Field Survey XVI. The angular momentum of low-mass star-forming galaxies. A cautionary tale and insights from TNG50
Nicolas F. Bouché, Shy Genel, Alisson Pellissier +14
We investigate the specific angular momentum (sAM) profiles of intermediate redshift () star-forming galaxies (SFGs) in the relatively unexplored regime of low…