The radio galaxy population in the SIMBA simulations
We examine the 1.4 GHz radio luminosities of galaxies arising from star formation and active galactic nuclei (AGNs) within the state-of-the-art cosmological hydrodynamic simulation SIMBA. SIMBA grows black holes via gravitational torque limited accretion from cold gas and Bondi accretion from hot ga...
| Main Authors: | , , , |
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| Format: | Journal article |
| Language: | English |
| Published: |
Royal Astronomical Society
2021
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