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Evidence of the fast acceleration of AGN-driven winds at kiloparsec scales - Nature Astronomy
Abstract Supermassive black holes at the centres of galaxies gain mass through accretion disks. Different models predict that quasi-spherical winds, expelled by black holes during accretion, have a key role in galaxy evolution through regulating star formation and the distribution of metals over kiloparsec scales and sweeping ambient gas to the outskirts of galaxies.
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