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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FR0 radio galaxy jets -- I. linking jet dynamics and high-energy emission in LEDA 55267 and LEDA 58287
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.