A Chandra Study of the Radio Galaxy NGC 326: Wings, Outburst History, and AGN Feedback

Abstract

NGC 326 is one of the most prominent X- or Z-shaped radio galaxies (XRGs/ZRGs) and has been the subject of several studies attempting to explain its morphology through either fluid motions or reorientation of the jet axis. We examine a 100 ks archival Chandra exposure and find several features associated with the radio galaxy: a high-temperature front that may indicate a shock, high-temperature knots around the rim of the radio emission, and a cavity associated with the eastern wing of the radio galaxy. A reasonable interpretation of these features in light of the radio data allows us to reconstruct the history of the AGN outbursts. The active outburst was likely once a powerful radio source which has since decayed, and circumstantial evidence favors reorientation as the means to produce the wings. Because of the obvious interaction between the radio galaxy and the ICM and the wide separation between the active lobes and wings, we conclude that XRGs are excellent sources in which to study AGN feedback in galaxy groups by measuring the heating rates associated with both active and passive heating mechanisms.

13 pages, 8 figures, Accepted by ApJ

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• Multi-frequency characterisation of remnant radio galaxies in the Lockman Hole field
• XMM-Newton Large Program on SN1006 - I: Methods and Initial Results of Spatially-Resolved Spectroscopy
• Dynamical Modelling and Emission Signatures of a Candidate Dual AGN with Precessing Radio Jets
• The physical structure of radio galaxies explored with three-dimensional simulations
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• Core prominence as a signature of restarted jet activity in the LOFAR radio-galaxy population