Deep LOFAR-VLBI imaging of the merging cluster Abell 2255 resolves, for the first time, thin non-thermal filaments 80 to 110 kpc long and 3 to 10 kpc wide in the tail of the Original Tailed Radio Galaxy.
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Revealing the intricacies of radio galaxies and filaments in the merging galaxy cluster Abell 2255. I. Insights from deep LOFAR-VLBI sub-arcsecond resolution images
Deep LOFAR-VLBI imaging of the merging cluster Abell 2255 resolves, for the first time, thin non-thermal filaments 80 to 110 kpc long and 3 to 10 kpc wide in the tail of the Original Tailed Radio Galaxy.