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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X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.
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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Investigating central star formation in local AGN host galaxies: is there tension between coeval growth and AGN feedback?
X-ray AGN fraction increases with central star formation rate density in local galaxies, supporting coeval black hole and galaxy growth with only modest time-averaged AGN feedback effects.