Radio jets clearing the way through galaxies: the view from HI and molecular gas
Raffaella Morganti (ASTRON, the Netherlands Institute for Radio, Astronomy, Kapteyn Astronomical Institute, University of Groningen)

TL;DR
This paper investigates how radio jets influence galaxy evolution by driving outflows of cold and molecular gas, using high-resolution observations to locate and analyze these interactions and their effects on the interstellar medium.
Contribution
It provides new high-resolution imaging evidence linking radio jets to cold gas outflows, supporting jet-driven outflow models and showing cold gas formation post-shock.
Findings
Radio jets are coincident with regions of cold gas outflows.
Cold gas can form after strong shocks and jet interactions.
Fast outflows are present even in weak radio sources.
Abstract
Massive gas outflows are considered a key component in the process of galaxy formation and evolution. Because of this, they are the topic of many studies aimed at learning more about their occurrence, location and physical conditions as well as the mechanism(s) at their origin. This contribution presents recent results on two of the best examples of jet-driven outflows traced by cold and molecular gas. Thanks to high-spatial resolution observations, we have been able to locate the region where the outflow occurs. This appears to be coincident with bright radio features and regions where the interaction between radio plasma jet and ISM is known to occur, thus strongly supporting the idea of jet-driven outflows. We have also imaged the distribution of the outflowing gas. The results clearly show the effect that expanding radio jets and lobes have on the ISM. This appears to be in good…
Peer Reviews
No public reviews on file for this paper yet. If you reviewed it on a platform where reviews are public (OpenReview, ICLR, NeurIPS, ICML), you can paste yours below so the community can read it here.
Videos
No videos yet. Explain this paper in a talk, walkthrough, or lecture? Add one.
