Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
M., Costa, T., Tadhunter, C
2 Pith papers cite this work. Polarity classification is still indexing.
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A low-luminosity AGN in ESO 420-G13 powers a jet-driven gas bubble and massive CO-dark molecular outflow with total kinetic power ~1.5e41 erg/s and ~3.8% coupling efficiency, expelling ~5% of the central molecular gas.
citing papers explorer
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AGN-driven outflows in dwarf galaxies from cosmological simulations: Internal properties and observational signatures
Cosmological zoom-in simulation of a 10^9.7 solar mass dwarf galaxy shows AGN outflows create >10^6 K bubbles accelerating gas to 600 km/s that recycle within 10 kpc, tracing observed BPT loci over time.
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Wild is the wind from low-luminosity AGN: a jet-driven gas bubble blowing out a massive CO-dark outflow in ESO 420-G13
A low-luminosity AGN in ESO 420-G13 powers a jet-driven gas bubble and massive CO-dark molecular outflow with total kinetic power ~1.5e41 erg/s and ~3.8% coupling efficiency, expelling ~5% of the central molecular gas.