CORDIS Project
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This project investigates how gas is transported to supermassive black holes in galaxies, focusing on the role of counter-rotating structures. It aims to understand the physical conditions that influence black hole feeding processes.
Supermassive black holes are ubiquitous in the centres of galaxies.
They remain largely invisible to our probes, except during their active phases (AGN), when gas is accreted onto the black hole.
The energy output of AGN is thought to be able to regulate the growth of galaxies and supermassive black holes.
However, we still do not understand how gas is transported to fuel the AGN.
One of the outstanding challenges in galaxy evolution is to uncover what physical conditions in the host galaxy trig…
KOBENHAVNS UNIVERSITET
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LOS ANGELES UCLA SANTA BARBARA UCSB DAVIS UCD RIVERSIDE UCR SAN DIEGO UCSD SANTA CRUZ UCSC IRVIN
United States, Berkeley
Type: University / higher education
Activity type: Higher or Secondary Education Establishments
SME: No
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