Evidence of strong quasar feedback in the early Universe

Abstract

Most theoretical models invoke quasar driven outflows to quench star formation in massive galaxies, this feedback mechanism is required to account for the population of old and passive galaxies observed in the local universe. The discovery of massive, old and passive galaxies at z=2, implies that such quasar feedback onto the host galaxy must have been at work very early on, close to the reionization epoch. We have observed the [CII]158um transition in SDSSJ114816.64+525150.3 that, at z=6.4189, is one of the most distant quasars known. We detect broad wings of the line tracing a quasar-driven massive outflow. This is the most distant massive outflow ever detected and is likely tracing the long sought quasar feedback, already at work in the early Universe. The outflow is marginally resolved on scales of about 16 kpc, implying that the outflow can really affect the whole galaxy, as required by quasar feedback models. The inferred outflow rate, dM/dt > 3500 Msun/yr, is the highest ever found. At this rate the outflow can clean the gas in the host galaxy, and therefore quench star formation, in a few million years.

5 pages, 3 figures, accepted for publication in MNRAS Letters

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• CO spectra of the ISM in the Host Galaxies of the Most Luminous WISE-Selected AGNs
• The EDGE-CALIFA survey: The effect of active galactic nucleus feedback on the integrated properties of galaxies at different stages of their evolution
• AGN radiative feedback in the early growth of massive black holes
• Impact of supermassive black hole growth on star formation
• ALMA uncovers optically thin and multi-component CO gas in the outflowing circumnuclear disk of NGC1068
• Broad [CII] line wings as tracer of molecular and multi-phase outflows in infrared bright galaxies
• Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
• Obscured accretion from AGN surveys
• Resolved Neutral Outflow from a Lensed Dusty Star Forming Galaxy at z=2.09
• Star Formation in Quasar Host Galaxies at Redshift 6: Millimeter Surveys and New Insights from ALMA
• The physical properties and impact of AGN outflows from high to low redshift
• Galaxy mergers can initiate quenching by unlocking an AGN-driven transformation of the baryon cycle
• Black Hole-Galaxy Correlations in Cluster Zoomed-in Simulations: GIZMO-SIMBA and TNG-Cluster
• The imprint of AGN-driven outflows on the CGM: the case of Lyα nebulae around high-z quasars
• Unveiling BLR Structure in AGN with High Resolution X-Ray Spectra: An Analytic Approach to Wind Emission Line Profiles
• Galaxy Activity, Torus and Outflow Survey (GATOS) X: Molecular gas clumpiness under the influence of AGN
• Entropy plateaus can emerge from gas replacement at a characteristic halo mass in simulated groups and clusters of galaxies
• On the quenching of star formation in observed and simulated central galaxies: Evidence for the role of integrated AGN feedback
• The AGN fuelling/feedback cycle in nearby radio galaxies -- IV. Molecular gas conditions and jet-ISM interaction in NGC3100
• The impact of black hole feedback on the UV luminosity and stellar mass assembly of high-redshift galaxies