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Cosmic Scale  /  Physics

Early quasars blast out kinetic energy at 260% of their total light output, effectively choking off the birth of new stars in their host galaxies.

JWST observations of the early universe reveal that these luminous objects produce galaxy-scale outflows at a rate nearly seven times higher than in later eras. These violent winds are powerful enough to strip gas from a galaxy before it can collapse into stars. Astronomers were puzzled by why some of the oldest galaxies in the universe stopped growing so suddenly. This data provides the first direct evidence of a cosmic 'off switch' that operates with extreme efficiency shortly after the Big Bang. This mechanism explains the existence of 'red and dead' galaxies that appear far earlier than standard models predicted. It shows that the early universe was far more violent than we ever imagined.

Original Paper

Frequent Extreme Galaxy-scale Outflows among Luminous Early Quasars

Weizhe Liu, Xiaohui Fan, Huan Li, Richard F Green, Jinyi Yang, Xiangyu Jin, Jianwei Lyu, Maria Anne Pudoka, Yongda Zhu, Eduardo Bañados, Silvia Belladitta, Thomas Connor, Tiago Costa, Anna-Christina Eilers, Hyunsung Jun, Madeline Marshall, Chiara Mazzucchelli, Jan-Torge Schindler, Yue Shen, Sylvain Veilleux, Julien Wolf, Huanian Zhang, Mingyang Zhuang, Siwei Zou, Mingyu Li

research_square  ·  rs-6674725

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), wit