Deep low-frequency radio observations of Abell 2256 I: The filamentary radio relic

TL;DR

This study provides detailed, multi-frequency radio images of Abell 2256's relic, revealing complex filamentary structures and a consistent power-law spectrum, enhancing understanding of shock acceleration in galaxy clusters.

Contribution

First spatially resolved spectral analysis of Abell 2256's relic across broad frequencies, confirming filamentary structures and shock-related acceleration processes.

Findings

Relic spectrum is a single power law with index -1.07 from 144 MHz to 3 GHz.

Filamentary substructures are confirmed at low frequencies.

Relic surface traces complex shock front with varying Mach numbers.

Abstract

We present deep and high fidelity images of the merging galaxy cluster Abell 2256 at low frequencies, using the upgraded Giant Metrewave Radio Telescope (uGMRT) and LOw-Frequency ARray (LOFAR). This cluster hosts one of the most prominent known relics, with a remarkably spectacular network of filamentary substructures. The new uGMRT (300-850 MHz) and LOFAR (120-169 MHz) observations, combined with the archival Karl G. Jansky Very Large Array (VLA; 1-4 GHz) data, allowed us to carry out the first spatially resolved spectral analysis of the exceptional relic emission down to 6 arcsec resolution over a broad range of frequencies. Our new sensitive radio images confirm the presence of complex filaments of magnetized relativistic plasma also at low frequencies. We find that the integrated spectrum of the relic is consistent with a single power law, without any sign of spectral steepening, at least below 3 GHz. Unlike previous claims, the relic shows an integrated spectral index of $-1.07\pm0.02$ between 144 MHz and 3 GHz, which is consistent with the (quasi)stationary shock approximation. The spatially resolved spectral analysis suggests that the relic surface very likely traces the complex shock front, with a broad distribution of Mach numbers propagating through a turbulent and dynamically active intracluster medium. Our results show that the northern part of the relic is seen edge-on and the southern part close to face-on. We suggest that the complex filaments are regions where higher Mach numbers dominate the (re-)acceleration of electrons that are responsible for the observed radio emission.