FIRE-3 cosmological simulations of Seyfert galaxies produce episodic AGN feedback and gas clearing but no clear anti-correlation between nuclear gas concentration and AGN luminosity, highlighting timing mismatches with observations.
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Simulation of barred galaxy shows inside-out NSD growth and shared NSC history regulated by feedback, indicating bar timescale and cluster accretion are key to nuclear scaling relations and favoring lower Milky Way bulge mass.
citing papers explorer
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Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations
FIRE-3 cosmological simulations of Seyfert galaxies produce episodic AGN feedback and gas clearing but no clear anti-correlation between nuclear gas concentration and AGN luminosity, highlighting timing mismatches with observations.
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SMUGGLE-Ring: Evolutionary link between nuclear star cluster and nuclear disk
Simulation of barred galaxy shows inside-out NSD growth and shared NSC history regulated by feedback, indicating bar timescale and cluster accretion are key to nuclear scaling relations and favoring lower Milky Way bulge mass.