Cold-gas outflows in typical low-redshift galaxies are driven by star formation, not AGN
Marc Sarzi, Sugata Kaviraj, Boris Nedelchev, Joshua Tiffany, Stanislav, S. Shabala, Adam T. Deller, Enno Middleberg

TL;DR
This study finds that in low-redshift galaxies, cold-gas outflows are primarily driven by star formation rather than AGN activity, with radio AGNs and outflows rarely occurring together.
Contribution
The paper provides observational evidence that cold-gas outflows in nearby galaxies are mainly caused by star formation, not AGN feedback, challenging assumptions about AGN-driven winds.
Findings
Cold-gas outflows are mostly associated with star-forming galaxies.
Radio AGNs are found mainly in early-type, gas-depleted galaxies.
No simultaneous evidence of radio AGN activity and cold-gas outflows was observed.
Abstract
Energetic feedback from active galactic nuclei (AGN) is an important ingredient for regulating the star-formation history of galaxies in models of galaxy formation, which makes it important to study how AGN feedback actually occurs in practice. In order to catch AGNs in the act of quenching star formation we have used the interstellar NaD absorption lines to look for cold-gas outflows in a sample of 456 nearby galaxies for which we could unambigously ascertain the presence of radio AGN activity, thanks to radio imaging at milli-arcsecond scales. While compact radio emission indicating a radio AGN was found in 103 galaxies (23% of the sample), and 23 objects (5%) exhibited NaD absorption-line kinematics suggestive of cold-gas outflows, not one object showed evidence of a radio AGN and of a cold-gas outflow simultaneously. Radio AGN activity was found predominantly in early-type galaxies,…
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