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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4 Pith papers cite this work, alongside 8 external citations. Polarity classification is still indexing.
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representative citing papers
New integral-field spectroscopy of quasar 3C 297 reveals an 18 kpc ionized gas outflow and jet-aligned young stars, interpreted as jet-dominated feedback in a merging host.
3D RHD simulations of FR0 jets in LEDA 55267 and LEDA 58287 show recollimation shocks driving compactness via turbulence and deceleration, with SED modeling predicting lepto-hadronic emission at TeV energies as a testable forecast.
A comprehensive review concludes that AGN jets couple strongly to the host ISM on kpc scales, driving multi-phase outflows, turbulence, and mixed suppression and enhancement of star formation.
citing papers explorer
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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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Mapping feedback signatures in 3C 297: A quasar-host merger at Cosmic Noon
New integral-field spectroscopy of quasar 3C 297 reveals an 18 kpc ionized gas outflow and jet-aligned young stars, interpreted as jet-dominated feedback in a merging host.
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Jet-Feedback on kpc scales: a review
A comprehensive review concludes that AGN jets couple strongly to the host ISM on kpc scales, driving multi-phase outflows, turbulence, and mixed suppression and enhancement of star formation.