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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2 Pith papers cite this work. Polarity classification is still indexing.
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Pith papers citing it
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2026 2verdicts
UNVERDICTED 2representative citing papers
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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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.