Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
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4 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 4verdicts
UNVERDICTED 4representative citing papers
Magnetic pressure up to 100 times gas pressure is required in AGN disks to sustain the longest inferred quasar lifetimes exceeding 10,000 years at high redshift.
Accretion feedback caps stellar growth rates below 0.1 solar masses per year in AGN disks, eliminates runaway accretion, and produces higher equilibrium masses and luminosities when gap opening is included.
Proximate damped Lyman-alpha systems trace cold dense gas participating in inflow-outflow cycles around quasars, supporting chaotic cold accretion scenarios.
citing papers explorer
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AGN-driven outflows in dwarf galaxies from cosmological simulations: Internal properties and observational signatures
Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
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The Lifetimes of High-redshift Quasars Suggest Magnetic Disk Support
Magnetic pressure up to 100 times gas pressure is required in AGN disks to sustain the longest inferred quasar lifetimes exceeding 10,000 years at high redshift.
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The Effects of Accretion Feedback on Stellar Evolution in AGN Disks
Accretion feedback caps stellar growth rates below 0.1 solar masses per year in AGN disks, eliminates runaway accretion, and produces higher equilibrium masses and luminosities when gap opening is included.
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Proximate damped Lyman-$\alpha$ systems as tracers of quasar feedback
Proximate damped Lyman-alpha systems trace cold dense gas participating in inflow-outflow cycles around quasars, supporting chaotic cold accretion scenarios.