AGN feedback from Jet-ISM/IGM interactions
V. Antonuccio-Delogu (Oxford, Catania), J. Silk (Oxford)
TL;DR
This paper models how relativistic jets from active galactic nuclei interact with their surrounding medium to suppress star formation within the galaxy.
Contribution
It introduces a new model linking AGN jet propagation to star formation suppression via cocoon expansion.
Findings
Jet-ISM/IGM interactions can significantly inhibit star formation.
The model predicts cocoon expansion impacts galaxy evolution.
Results align with observed galaxy quenching phenomena.
Abstract
We study the propagation of relativistic jets originating from AGNs within the Interstellar/Intergalactic Medium of their host galaxies, and use it to build a model for the suppression of stellar formation within the expanding cocoon.
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