Extreme Galaxy-scale Outflows Are Frequent among Luminous Early Quasars
arXiv:2509.08793 · doi:10.1038/s41586-026-10477-9
Abstract
The existence of abundant post-starburst/quiescent galaxies just 1-2 Gyrs after the Big Bang challenges our current paradigm of galaxy evolution. Cosmological simulations suggest that quasar feedback is likely the most promising mechanism responsible for such rapid quenching. Here we report a high detection rate (6/27) of exceptionally fast and powerful galaxy-scale outflows traced by [O III] emission in z 5-6 luminous quasars as revealed by the James Webb Space Telescope (JWST), with velocity up to 8400 km s and order-of-magnitude kinetic energy outflow rates up to 260% the observed quasar bolometric luminosities. This fraction is 3.9 and 8.8 times of those in comparison samples at z 1.5-3.5 and z 1, respectively. These extreme outflows are comparable to or even faster than the most rapid [O III] outflows reported at z 3, and could reach the circumgalactic medium (CGM) or even the intergalactic medium (IGM). The average kinetic energy outflow rate of our sample is more than 2 dex higher than those of the lower-redshift comparison samples. The substantially higher frequency of outflows with energetics well above the threshold for negative feedback in our sample strongly suggests that quasar feedback plays a significant role in efficiently quenching/regulating early massive galaxies.
27 pages, 8 figures, 2 tables. Final version published in Nature at https://www.nature.com/articles/s41586-026-10477-9
References in corpus (33)
- galpy: A Python Library for Galactic Dynamics
- The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope I. Overview of the instrument and its capabilities
- The Sloan Digital Sky Survey Quasar Catalog: Sixteenth Data Release
- Kiloparsec-scale outflows are prevalent among luminous AGN: outflows and feedback in the context of the overall AGN population
- A massive quiescent galaxy at redshift 4.658
- An Atlas of Color-selected Quiescent Galaxies at in Public Fields
- The WISSH Quasars Project I. Powerful ionised outflows in hyper-luminous quasars
- The Near-Infrared Spectrograph (NIRSpec) on the James Webb Space Telescope III. Integral-field spectroscopy
- A Catalog of Quasar Properties from Sloan Digital Sky Survey Data Release 16
- A 3D Drizzle Algorithm for JWST and Practical Application to the MIRI Medium Resolution Spectrometer
- A massive galaxy that formed its stars at
- Extremely Red Quasars in BOSS
- The REQUIEM Survey I: A Search for Extended Ly-Alpha Nebular Emission Around 31 z>5.7 Quasars
- EIGER V. Characterizing the Host Galaxies of Luminous Quasars at
- A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): JWST Reveals a Filamentary Structure around a z=6.61 Quasar
- A survey of luminous high-redshift quasars with SDSS and WISE II. the bright end of the quasar luminosity function at z ~ 5
- A SPectroscopic survey of biased halos In the Reionization Era (ASPIRE): A First Look at the Rest-frame Optical Spectra of Quasars Using JWST
- Widespread, strong outflows in XQR-30 quasars at the Reionisation epoch
- No evidence for [CII] halos or high-velocity outflows in z>6 quasar host galaxies
- GA-NIFS: Black hole and host galaxy properties of two z6.8 quasars from the NIRSpec IFU
- Physical constraints on the extended interstellar medium of the z=6.42 quasar J1148+5251: [CII] 158um, [NII] 205um and [OI] 146um observations
- AGN-driven outflows and the formation of Ly nebulae around high-z quasars
- Orientation effects on spectral emission features of quasars
- First results from the JWST Early Release Science Program Q3D: The Warm Ionized Gas Outflow in z ~ 1.6 Quasar XID 2028 and its Impact on the Host Galaxy
- Integral-Field Spectroscopy of Fast Outflows in Dwarf Galaxies with AGN
- A quasar-galaxy merger at : black hole mass and quasar properties from the NIRSpec spectrum
- The First Quiescent Galaxies in TNG300
- ALMA Observations of Quasar Host Galaxies at
- A quasar-galaxy merger at : rapid host growth via accretion of two massive satellite galaxies
- High-redshift quasars and their host galaxies II: multiphase gas and stellar kinematics
- JADES: Rest-frame UV-to-NIR Size Evolution of Massive Quiescent Galaxies from Redshift z=5 to z=0.5
- Fading Light, Fierce Winds: JWST Snapshot of a Sub-Eddington Quasar at Cosmic Dawn
- JWST's PEARLS: A z=6 quasar in a train-wreck galaxy merger system