Another shock for the Bullet cluster, and the source of seed electrons for radio relics
Timothy W. Shimwell, Maxim Markevitch, Shea Brown, Luigina Feretti, B., M. Gaensler, M. Johnston-Hollitt, Craig Lage, Raghav Srinivasan

TL;DR
This study reports a new radio relic in the Bullet cluster, linked to a shock front and likely originating from a nearby radio galaxy remnant, providing insights into relic formation mechanisms.
Contribution
It presents the discovery of a highly luminous radio relic with a coincident X-ray shock, suggesting a novel seed electron source from a local radio galaxy remnant.
Findings
The relic is the brightest known with a surface brightness of 94% of total flux.
A shock front is identified coincident with the relic, supporting shock re-acceleration models.
Seed electrons may originate from a local radio galaxy remnant, not uniformly mixed in the ICM.
Abstract
With Australia Telescope Compact Array observations, we detect a highly elongated Mpc-scale diffuse radio source on the eastern periphery of the Bullet cluster 1E0657-55.8, which we argue has the positional, spectral and polarimetric characteristics of a radio relic. This powerful relic (2.3+/-0.1 x 10^25 W Hz^-1) consists of a bright northern bulb and a faint linear tail. The bulb emits 94% of the observed radio flux and has the highest surface brightness of any known relic. Exactly coincident with the linear tail we find a sharp X-ray surface brightness edge in the deep Chandra image of the cluster -- a signature of a shock front in the hot intracluster medium (ICM), located on the opposite side of the cluster to the famous bow shock. This new example of an X-ray shock coincident with a relic further supports the hypothesis that shocks in the outer regions of clusters can form relics…
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