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Restarting activity in the nucleus of PBC J2333.9-2343: An extreme case of jet realignment

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TLDR
In this article, the spectral energy distribution (SED) of the radio galaxy PBC J2333.9-2343 was analyzed using simultaneous multi-wavelength data from the Very Long Baseline Array (VLBA), the San Pedro Martir telescope, and the XMM-Newton observatories.
Abstract
Context. The giant radio galaxy PBC J2333.9-2343 shows different characteristics at different wavebands that are difficult to explain within the actual generic schemes of unification of active galactic nuclei (AGN). It is therefore a good candidate host for different phases of nuclear activity. Aims. We aim at disentangling the nature of this AGN by using simultaneous multiwavelength data. Methods. We obtained data in 2015 from the Very Long Baseline Array (VLBA), the San Pedro Martir telescope, and the XMM-Newton observatories. This allows the study of the nuclear parts of the galaxy through its morphology and spectra and the analysis of the spectral energy distribution (SED). We also reanalysed previously-presented optical data from the San Pedro Martir telescope from 2009 to provide a homogeneous comparison. Results. At X-ray frequencies the source is unabsorbed. The optical spectra are of a type 1.9 AGN, both in 2009 and 2015, although showing a broader component in 2015. The VLBA radio images show an inverted spectrum with a self-absorbed, optically thick compact core ( α c = 0.40, where S ν ∝ ν + α ) and a steep-spectrum, optically thin jet ( α j,8−15 = −0.5). The SED resembles that of typical blazars and is best represented by an external Compton (EC) model with a viewing angle of approximately 3–6°. The apparent size of the large-scale structure of PBC J2333.9-2343 must correspond to an intrinsic deprojected value of approximately 7 Mpc for θ v 13 Mpc for θ v Conclusions. The above arguments suggest that PBC J2333.9-2343 has undergone a new episode of nuclear activity and that the direction of the new jet has changed in the plane of the sky and is now pointing towards us. This changes this source from a radio galaxy to a blazar, a very exceptional case of restarting activity.

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The Fourth Catalog of Active Galactic Nuclei Detected by the Fermi Large Area Telescope

Marco Ajello, +152 more
TL;DR: The 4LAC catalog of active galactic nuclei (AGNs) detected by the Fermi Gamma-ray Space Telescope Large Area Telescope (4LAC) between 2008 August 4 and 2016 August 2 contains 2863 objects located at high Galactic latitudes (|b|>10°deg}).
Journal ArticleDOI

Hard X-ray-selected giant radio galaxies - I. The X-ray properties and radio connection

TL;DR: In this paper, a broad-band X-ray study of the nuclei of 14 hard-X-ray-selected giant radio galaxies is presented, based both on the literature and on the analysis of archival X-Ray data from NuSTAR, XMM-Newton, Swift, and INTEGRAL.
Journal ArticleDOI

Hard X-ray selected giant radio galaxies - II. Morphological evidence of restarted radio activity

TL;DR: In this article, the authors presented a radio morphological study of a sample of 15 hard X-ray selected GRG, discussing low-frequency images from our GMRT campaign complemented with others from the literature: among them, 7/15 show evidence of restarted radio activity either in the form of double-double/X-shaped morphology, or as a cocoon emission embedding more recent jets.
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