The `Main' galaxy cluster in the Abell 781 system is undergoing a significant merger and accretion process with peripheral emission to the north and southeastern flanks of the merging structure. Here we present a full polarimetric study of this field, using radio interferometric data taken at 21 and 92 cm with the Westerbork Synthesis Radio Telescope, to a sensitivity better than any 21 cm (L-band) observation to date. We detect evidence of extended low-level emission of 1.9 mJy associated with the Main cluster at 21 cm, although this detection necessitates further follow-up by modern instruments due to the limited resolution of the Westerbork Synthesis Radio Telescope. Our polarimetric study indicates that, most likely, the peripheral emission associated with this cluster is not a radio relic.
@article{arxiv.2309.09909,
title = {Radio multifrequency observations of Abell~781 with the WSRT},
author = {B. V. Hugo and G. Bernardi and O. M. Smirnov and D. Dallacasa and T. Venturi and M. Murgia and R. F. Pizzo},
journal= {arXiv preprint arXiv:2309.09909},
year = {2023}
}