A Dissection of Spatially Resolved AGN Feedback across the
  Electromagnetic Spectrum
  We present optical SuperNova Integral Field Spectrograph (SNIFS) integral
field spectroscopy, Hubble Space Telescope optical imaging, Chandra X-ray
imaging, and Very Large Array radio interferometry of the merging galaxy 2MASX
J04234080+0408017, which hosts a Seyfert 2 active galactic nucleus (AGN) at z =
0.046. Our observations reveal that radiatively driven, ionized gas outflows
are successful to distances > 10 kpc due to the low mass of the host system,
encompassing the entirety of the observed optical emission. We also find that
at large radii, where observed velocities cannot be reproduced by radiative
driving models, high velocity kinematics are likely due to mechanical driving
from AGN winds impacting high density host material. This impacting deposits
sufficient energy to shock the host material, producing thermal X-ray emission
and cosmic rays, which in turn promote the formation of in situ radio structure
in a pseudo-jet morphology along the high density lanes.
