franco_vazzaBeautiful relativistic MHD simulations of the initial stage of jets expansion, as a function of their different orientation with respect to the main axis of the halo of their host galaxy.
New simulations using the PLUTO code by G. Giri and collaborators today on #astroph
https://arxiv.org/abs/2604.05471
"Galactic-scale evolution of classical and complex radio galaxies. Impact of ambient morphology and jet geometry"
