This process is experimental and the keywords may be updated as the learning algorithm improves.Īlexander, D. M., & Hickox, R. C.
These keywords were added by machine and not by the authors. Our study highlights that even when a quasar is formally “radio-quiet” the radio emission can be extremely effective for observing the effects of AGN feedback. Furthermore, their appears to be a large amount of mechanical energy input from this AGN, despite it being formally “radio quiet”. These observations show that the AGN is interacting with the interstellar medium across multiple scales. We observe \(\approx \)10–12 kpc radio bubbles each side of the nucleus, the larger of which is associated with an arc of luminous ionised gas, which appear to be inflated by the central AGN. This is likely to be a radio jet driving the outflow or a quasar wind that is shocking the ISM at this position. In the central \(\approx \)1 kpc we observe a high-velocity ionised outflow that is co-spatial with a radio structure. In this chapter we aim to address the question: what is the physical connection between the radio emission and ionised gas kinematics in radio-quiet quasars? In this pilot study, we present VLA radio and VIMOS IFU observations of the radio-quiet, type 2 quasar that has been nicknamed the “Teacup AGN” due to it emission-line region morphology.