WISE J233237.05-505643.5: a Double-Peaked Broad-Lined AGN with
  Spiral-Shaped Radio Morphology
  We present radio continuum mapping, optical imaging and spectroscopy of the
newly discovered double-peaked broad-lined AGN WISE J233237.05-505643.5 at
redshift z = 0.3447. This source exhibits an FR-I and FR-II hybrid-morphology,
characterized by bright core, jet, and Doppler-boosted lobe structures in ATCA
continuum maps at 1.5, 5.6, and 9 GHz. Unlike most FR-II objects, W2332-5056 is
hosted by a disk-like galaxy. The core has a projected 5" linear radio feature
that is perpendicular to the curved primary jet, hinting at unusual and complex
activity within the inner 25 kpc. The multi-epoch optical-near-IR photometric
measurements indicate significant variability over a 3-20 year baseline from
the AGN component. Gemini-South optical data shows an unusual double-peaked
emission-line features: the centroids of the broad-lined components of H-alpha
and H-beta are blueshifted with respect to the narrow lines and host galaxy by
~ 3800 km/s. We examine possible cases which involve single or double
supermassive black holes in the system, and discuss required future
investigations to disentangle the mystery nature of this system.
