Radio AGN feedback sustains quiescence only in a minority of massive galaxies

TL;DR

This study uses AI to distinguish galaxies where radio AGN feedback effectively prevents gas cooling from those where it does not, revealing that only a minority of massive galaxies are significantly influenced by radio AGNs.

Contribution

Introduces an AI-based method to classify galaxies by radio feedback effectiveness, challenging the assumption that radio AGNs universally maintain galaxy quiescence.

Findings

RFE galaxies are all dynamically hot with little cold gas.

RFI-Q galaxies often have substantial cold gas and extended disks.

Most RFE galaxies have experienced multiple radio feedback cycles.

Abstract

Radio active galactic nuclei (AGNs) eject a huge amount of energy into the surrounding medium and are thought to potentially prevent gas cooling and maintain the quiescence of massive galaxies. The short-lived, sporadic, and anisotropic nature of radio activities, coupled with the detection of abundant cold gas around some massive quiescent galaxies, raise questions about the efficiency of radio feedback in massive galaxies. Here we present an innovative method rooted in artificial intelligence to separate galaxies in which radio feedback is effective (RFE), regardless of current radio emission, from those in which radio feedback is ineffective (RFI), according to their optical images. Galaxies categorized as RFE are all dynamically hot, whereas quiescent RFI (RFI-Q) galaxies usually have extended cold-disk components. At given stellar mass, dark matter halos hosting RFE galaxies are between four to ten times more massive than those of RFI-Q galaxies. We find, for the first time, that almost all RFE galaxies have scant cold gas, irrespective of AGN activity. In contrast, many RFI-Q galaxies are surrounded by substantial amounts of condensed atomic gas, indicating a different evolutionary path from RFE galaxies. Our finding provides direct and compelling evidence that a radio AGN has gone through about 300 on-off cycles and that radio feedback can prevent gas cooling over a timescale much longer than that of radio activity. Contrary to general belief, our analysis shows that only a small fraction of massive galaxies are influenced by strong radio AGNs, suggesting that current galaxy formation models need serious revision.