Jet Feedback in Star-Forming Galaxies

In this paper, I review our understanding of how jet feedback works in star-forming galaxies. There are some interesting differences to radiative from Active Galactic Nuclei (AGN). Jets act on galaxy haloes as well dense gas, for example regularly rotating discs, where they can suppress star formation (particularly the centre, negative feedback), but also enhance it (positive feedback). Jet may produce turbulent, multi-phase gas structures shocks contribute ionisation and is observed connection with galactic outflows. The exact driving mechanism these outflows still unclear, be a combination effects linked formation, jet-induced turbulence AGN feedback. Supermassive black holes any jets. Preferential radio detections more massive galaxies explained different conditions circumgalactic medium and, correspondingly, jet–environment interactions.