Fully cosmological virtual massive galaxies at z = 0: kinematical, morphological and stellar population characterization
We present the results of a numerical adaptive mesh refinement hydrodynamical and N-body simulation in a Λ cold dark matter cosmology. We focus on the analysis of the main properties of massive galaxies (M* > 1011 M⊙) at z = 0. For all the massive virtual galaxies, we carry out a careful study of their one-dimensional density, luminosity, velocity
Vazdekis, A. et al.
Advertised on:
12
2013