Ram pressure feeding super-massive black holes
Bianca M. Poggianti, Yara L. Jaff\'e, Alessia Moretti, Marco, Gullieuszik, Mario Radovich, Stephanie Tonnesen, Jacopo Fritz, Daniela, Bettoni, Benedetta Vulcani, Giovanni Fasano, Callum Bellhouse, George Hau,, Alessandro Omizzolo

TL;DR
This study reveals a strong link between ram pressure stripping in galaxy clusters and the activation of supermassive black holes as AGN, suggesting ram pressure as a novel mechanism for fueling black hole accretion.
Contribution
It demonstrates that ram pressure stripping can funnel gas towards galaxy centers, potentially triggering AGN activity, a previously underappreciated feeding mechanism.
Findings
6 out of 7 jellyfish galaxies host AGN
Two galaxies show galactic-scale ionization cones
Galaxy position and velocity support ram pressure as feeding mechanism
Abstract
When supermassive black holes at the center of galaxies accrete matter (usually gas), they give rise to highly energetic phenomena named Active Galactic Nuclei (AGN). A number of physical processes have been proposed to account for the funneling of gas towards the galaxy centers to feed the AGN. There are also several physical processes that can strip gas from a galaxy, and one of them is ram pressure stripping in galaxy clusters due to the hot and dense gas filling the space between galaxies. We report the discovery of a strong connection between severe ram pressure stripping and the presence of AGN activity. Searching in galaxy clusters at low redshift, we have selected the most extreme examples of jellyfish galaxies, which are galaxies with long tentacles of material extending for dozens of kpc beyond the galaxy disk. Using the MUSE spectrograph on the ESO Very Large Telescope, we…
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