Supernova-driven galactic winds fall into three regimes set by the ratio of supernova scale height to gas scale height, which controls how much mass, metals, and energy escape.
Large-scale Fountains around a Milky Way-like Galaxy
3 Pith papers cite this work, alongside 49 external citations. Polarity classification is still indexing.
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astro-ph.GA 3representative citing papers
TNG50 MW analogues reproduce global soft X-ray luminosity, inner surface brightness, emission measure and O VII absorption but show too-steep radial decline in X-ray brightness and 65% lower O VIII absorption than observed, indicating overly central feedback.
FIRE-3 cosmological simulations of Seyfert galaxies produce episodic AGN feedback and gas clearing but no clear anti-correlation between nuclear gas concentration and AGN luminosity, highlighting timing mismatches with observations.
citing papers explorer
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QUOKKA-based understanding of outflows (QED) -- III. Outflow loading and phase structure as a function of galactic environment
Supernova-driven galactic winds fall into three regimes set by the ratio of supernova scale height to gas scale height, which controls how much mass, metals, and energy escape.
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Probing the Hot Gaseous Halos of Milky Way-like Galaxies in the TNG50 simulation
TNG50 MW analogues reproduce global soft X-ray luminosity, inner surface brightness, emission measure and O VII absorption but show too-steep radial decline in X-ray brightness and 65% lower O VIII absorption than observed, indicating overly central feedback.
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Investigating black hole accretion and feedback self-regulation in Seyfert galaxies using the FIRE-3 cosmological hydrodynamic simulations
FIRE-3 cosmological simulations of Seyfert galaxies produce episodic AGN feedback and gas clearing but no clear anti-correlation between nuclear gas concentration and AGN luminosity, highlighting timing mismatches with observations.