The deepest $Chandra$ view of RBS 797: evidence for two pairs of equidistant X-ray cavities
Francesco Ubertosi, Myriam Gitti, Fabrizio Brighenti, Gianfranco, Brunetti, Michael McDonald, Paul Nulsen, Brian McNamara, Scott Randall,, William Forman, Megan Donahue, Alessandro Ignesti, Massimo Gaspari, Stefano, Ettori, Luigina Feretti, Elizabeth L. Blanton, Christine Jones

TL;DR
This study presents the discovery of four symmetric X-ray cavities in galaxy cluster RBS 797, indicating complex AGN activity with possible binary black holes or rapid jet reorientation.
Contribution
First deep Chandra observation revealing four equidistant, radio-filled cavities in RBS 797, suggesting dual outbursts or jet reorientation.
Findings
Detection of two additional N-S cavities at similar radii as E-W cavities.
Cavities are associated with radio emission at 1.4 and 4.8 GHz.
Estimated ages of cavities indicate nearly simultaneous outbursts.
Abstract
We present the first results of a deep observation of the galaxy cluster RBS 797, whose previous X-ray studies revealed two pronounced X-ray cavities in the east-west (E-W) direction. Follow-up VLA radio observations of the central active galactic nucleus (AGN) uncovered different jet and lobe orientations, with radio lobes filling the E-W cavities and perpendicular jets showing emission in the north-south (N-S) direction over the same scale (30 kpc). With the new 427 ks total exposure, we report the detection of two additional, symmetric X-ray cavities in the N-S direction at nearly the same radial distance as the E-W ones. The newly discovered N-S cavities are associated with the radio emission detected at 1.4 GHz and 4.8 GHz in archival VLA data, making RBS 797 the first galaxy cluster found to have four equidistant, centrally-symmetric, radio-filled…
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