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.
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2 Pith papers cite this work. Polarity classification is still indexing.
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Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.
citing papers explorer
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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.
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Very High Energy Gamma Rays from Ultra Fast Outflows
Several nearby AGN ultra-fast outflows are predicted to produce detectable very-high-energy gamma rays via shock-accelerated protons, visible to CTAO even if invisible to Fermi-LAT.