Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
Populating a cluster of galaxies - I. Results at \fontshape{it}{z}=0
We simulate the assembly of a massive rich cluster and the formation of its constituent galaxies in a flat, low-density universe. Our most accurate model follows the collapse, the star formation history and the orbital motion of all galaxies more luminous than the Fornax dwarf spheroidal, while dark halo structure …