83 citations · 306 across the 11 of their papers we have counts for
6 papers · 1 filter
On the redshift evolution of the baryon and gas fraction in simulated groups and clusters of galaxies
M. Angelinelli, S. Ettori, K. Dolag +2
We study the redshift evolution of the baryon budget in a large set of galaxy clusters from the {\it Magneticum} suite of SPH cosmological simulations. At high redshifts, we obtain…
Magnetogenesis and the Cosmic Web: a joint challenge for radio observations and numerical simulations
Franco Vazza, Nicola Locatelli, Kamlesh Rajpurohit +16
The detection of the radio signal from filaments in the cosmic web is crucial to distinguish possible magnetogenesis scenarios. We review the status of the different attempts to de…
Properties of clumps and filaments around galaxy clusters
M. Angelinelli, S. Ettori, F. Vazza +1
We report on the possibility of studying the proprieties of cosmic diffuse baryons by studying self-gravitating clumps and filaments connected to galaxy clusters. While filaments a…
Turbulent pressure support and hydrostatic mass-bias in the intracluster medium
M. Angelinelli, F. Vazza, C. Giocoli +5
The degree of turbulent pressure support by residual gas motions in galaxy clusters is not well known. Mass modelling of combined X-ray and Sunyaev Zel'dovich observations provides…
Detecting shocked intergalactic gas with X-ray and radio observations
F. Vazza, S. Ettori, M. Roncarelli +3
Detecting the thermal and non-thermal emission from the shocked cosmic gas surrounding large-scale structures represents a challenge for observations, as well as a unique window in…
The turbulent pressure support in galaxy clusters revisited
F. Vazza, M. Angelinelli, T. W. Jones +4
Due to their late formation in cosmic history, clusters of galaxies are not fully in hydrostatic equilibrium and the gravitational pull of their mass at a given radius is expected…