MOSCARDINI , L.

We model the cosmological co-evolution of galaxies and their central supermassive black holes (BHs) within a semi-analytical framework developed on the outputs of the Millennium Simulation citep{croton2006,delucia2007}. In this work, we analyze the model BH scaling relations, fundamental plane and mass function, and compare them with the most...

We model the cosmological co-evolution of galaxies and their central supermassive black holes (BHs) within a semi-analytical framework developed on the outputs of the Millennium Simulation. This model, described in detail by Croton et al. and De Lucia and Blaizot, introduces a `radio mode' feedback from AGN at the centre of X-ray emitting...