Compact radio sources: Triggering and feedback

CSS/GPS objects represent a key stage in the evolution of powerful radio AGN which jets are expanding through denser, kpc-scale ISM host galaxies. Therefore, it is important both to understand how such triggered as galaxies evolve and directly quantify impact outflows induced by jet-cloud interactions. Here, we show that sources likely be galaxy mergers, just like general. However, they more gas-rich have higher star formation rates on average than their extended counterparts. Also, whereas observations frequently evidence for strong interactions form warm outflows, most cases these unlikely energetic enough affect histories entire outside central kpc. Rather, much mass, energy, momentum appear tied up neutral molecular may Finally, consider whether impostors flux-limited samples due effect luminosities.