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Pressure of the hot gas in simulations of galaxy clusters
S. Planelles, D. Fabjan, S. Borgani +11
We analyze the radial pressure profiles, the ICM clumping factor and the Sunyaev-Zel'dovich (SZ) scaling relations of a sample of simulated galaxy clusters and groups identified in…
NIHAO XIII: Clumpy discs or clumpy light in high redshift galaxies?
Tobias Buck, Andrea V. Macciò, Aura Obreja +3
Many massive star forming disc galaxies in the redshift range 3 to 0.5 are observed to have a clumpy morphology showing giant clumps of size 1 kpc and masses of about $10^7M_…
Panchromatic Spectral Energy Distributions of simulated galaxies: results at redshift
David Goz, Pierluigi Monaco, Gian Luigi Granato +5
We present predictions of Spectral Energy Distributions (SEDs), from the UV to the FIR, of simulated galaxies at . These were obtained by post-processing the results of an N-b…
Kinetic AGN Feedback Effects on Cluster Cool Cores Simulated using SPH
Paramita Barai, Giuseppe Murante, Stefano Borgani +4
We implement novel numerical models of AGN feedback in the SPH code GADGET-3, where the energy from a supermassive black hole (BH) is coupled to the surrounding gas in the kinetic…