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.
Observing positive and negative AGN feedback
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abstract
Galaxy-scale outflows powered by actively accreting supermassive black holes are routinely detected, and they have been associated both with suppression and triggering of star formation. Recent observational evidence and simulations are favouring a delayed mechanism that connects outflows and star formation
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astro-ph.GA 2years
2026 2verdicts
UNVERDICTED 2representative citing papers
Proposal for statistical study of AGN outflows at cosmic noon using adaptive-optics 3D spectroscopy to map outflow rates and SFR without geometry assumptions.
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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SUNRISE-3D: Sharp UNveiling of AGN feedback Regulation and its Impact on Star-formation at the cosmic noon Epoch
Proposal for statistical study of AGN outflows at cosmic noon using adaptive-optics 3D spectroscopy to map outflow rates and SFR without geometry assumptions.