arXiv · 1310.2257
WISE J233237.05-505643.5: a Double-Peaked Broad-Lined AGN with Spiral-Shaped Radio Morphology
Abstract
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.
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Chao-Wei Tsai, Thomas H. Jarrett, Daniel Stern, Emonts Bjorn, R. Scott Barrows, Roberto J. Assef, Ray P. Norris, Peter R. M. Eisenhardt, Carol J. Lonsdale, Andrew W. Blain, Dominic J. Benford, Jingwen Wu, Brian Stalder, Christopher W. Stubbs, F. William High, K. L. Li, Albert K. H. Kong. 2013-10-08. WISE J233237.05-505643.5: a Double-Peaked Broad-Lined AGN with Spiral-Shaped Radio Morphology. https://doi.org/10.1088/0004-637x%2F779%2F1%2F41
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