JWST-NIRSpec data reveal AGN photoionization dominating gas excitation within 300 pc of NGC7469's nucleus, with shock signatures from a compact radio jet and complex kinematics indicating inflows and outflows in a self-regulating cycle.
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ArkenstoneBH is a new subgrid model for the hot phase of black hole feedback that, in isolated galaxy tests, suppresses star formation by counteracting gas inflows from the circumgalactic medium.
Radio AGN jets inject a total kinetic power density of 10^32 to 10^33 W per cubic megaparsec from z=0 to 2.5, matching requirements for feedback in galaxy evolution models.
citing papers explorer
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GOALS-JWST: Gas Dynamics and Excitation in NGC7469 revealed by NIRSpec
JWST-NIRSpec data reveal AGN photoionization dominating gas excitation within 300 pc of NGC7469's nucleus, with shock signatures from a compact radio jet and complex kinematics indicating inflows and outflows in a self-regulating cycle.
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ArkenstoneBH. A model for high-specific energy black hole feedback in cosmological simulations
ArkenstoneBH is a new subgrid model for the hot phase of black hole feedback that, in isolated galaxy tests, suppresses star formation by counteracting gas inflows from the circumgalactic medium.
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A population-based approach to understanding radio AGN feedback with LOFAR: The LoTSS Deep Fields
Radio AGN jets inject a total kinetic power density of 10^32 to 10^33 W per cubic megaparsec from z=0 to 2.5, matching requirements for feedback in galaxy evolution models.