The role of AGN feedback on the evolution of dwarf galaxies from cosmological simulations: SMBHs suppress star formation in low-mass galaxies
arxiv(2024)
摘要
Aims. Recent observational studies suggest that feedback from active galactic
nuclei (AGNs) may play an important role in the formation and evolution of
low-mass dwarf galaxies, an issue that has received little attention from a
theoretical perspective. Methods. We investigate this using two sets of 12
cosmological magneto-hydrodynamical simulations of the formation of dwarf
galaxies: one set using a version of the AURIGA galaxy formation physics model
including AGN feedback and a parallel set with AGN feedback turned off.
Results. We show that the full-physics AGN runs satisfactorily reproduce
several scaling relations, including the M_ BH-M_*, M_ BH-sigma_* and the
baryonic Tully-Fisher relation. We find that the global star formation (SF) of
galaxies run with AGN is reduced compared to the one in which AGN has been
turned off, suggesting that this type of feedback is a viable way of
suppressing SF in low-mass dwarfs, even though none of our galaxies is
completely quenched by z=0. Furthermore, we found a tight correlation between
the median SF rates and the black-hole-to-stellar mass ratio (M_BH/M_star) in
our simulated dwarfs. SF is suppressed due to gas heating in the vicinity of
the AGN: less HI gas is available in AGN runs, though the total amount of gas
is preserved across the two settings within each galaxy. This indicates that
the main effect of AGN feedback in our dwarfs is to heat up and push the gas
away from the galaxy's centre rather than expelling it completely. Finally, we
show that the two galaxies harbouring the largest BHs have suffered a
considerable (up to 65
pinpointing the role of AGNs in determining the final dark matter mass
distribution within dwarf galaxies. This pilot paper highlights the importance
of modelling AGN feedback at the lowest mass scales and the impact this can
have on dwarf galaxy evolution.
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