CORDIS Project
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This project explores the feedback mechanisms of supermassive black holes on galaxy evolution, focusing on how energy is released and its impact on surrounding environments. It aims to develop models that connect microphysical processes to galactic-scale phenomena.
It is firmly established that supermassive black holes (SMBHs) have a profound influence on the evolution of galaxies and galaxy groups/clusters.
Yet, almost 20 years after this realization, fundamental questions remain.
What determines the efficiency with which an active galactic nucleus (AGN) couples to its surroundings?
Why does AGN feedback appear to be ineffective in low-mass galaxies?
In maintenance-mode feedback, how does the AGN regulate to closely balance cooling?
How does the nature of…
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