Determining the full satellite population of a Milky Way-mass halo in a highly resolved cosmological hydrodynamic simulation
            
    We investigate the formation of the satellite galaxy population of a Milky Way-mass halo in a very highly resolved magnetohydrodynamic cosmological zoom-in simulation (baryonic mass resolution m b = 800 $\rm M_{\odot }$). We show that the properties of the central star-forming galaxy, such as the radial stellar surface density profile and star
            Grand, Robert J. J. et al.
Fecha de publicación:
11
            
                        2021