The interplay between radio jets and ISM in sub-kpc radio sources

Understand

This paper reviews the evidence for interaction between radio jets and their environment in small and intermediate (sub-kpc) scale radio sources.

• Observations of gas (both neutral hydrogen and ionised gas) have shown the presence of fast (> 1000 km/s) outflows likely originating from this interaction.
• The characteristics of these AGN-driven outflows (e.g.
• mass outflow rate) indicate that they may have a relevant impact on the evolution of the host galaxy.