We investigate the environmental properties of the = 0 radio galaxy population using the simba cosmological hydrodynamic simulation. We identify centrals and satellites from a population of high and low excitation radio galaxies (HERGs and LERGs) in simba, and study their global properties. We find that [Formula: see text] of radio galaxies are satellites, and that there are insignificant differences in the global properties of LERGs based on their central/satellite classification.
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