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.
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11
2021