A LOFAR view into the stormy environment of the galaxy cluster 2A0335+096

Context. Radio observations represent a powerful probe of the physics occurring in intracluster medium (ICM) because they trace relativistic cosmic rays cluster magnetic fields, or within galaxies themselves. By probing low-energy rays, low-frequency radio are especially interesting unveil emission powered by low-efficiency particle acceleration processes, which believed to play crucial role origin diffuse emission. Aims. We investigate mini-halo at centre galaxy 2A0335+096 and its connection central sloshing cool core. also study properties head-tail GB6 B0335+096 hosted explore life cycle electrons tails. Methods. used new LOw Frequency ARray (LOFAR) from LOFAR Two-meter Sky Survey 144 MHz map with high level detail. The data were combined archival Giant Metrewave Telescope Chandra carry out multi-wavelength study. Results. have made first measurement spectral index ( ? = ?1.2 ± 0.1 between 1.4 GHz) lobes source ? ?1.5 610 MHz). Based on morphology respect thermal ICM, we propose that is linked reveal presence megaparsec-long tail associated B0335+096. observed projected length factor 3 longer than expected cooling length, evidence flattening trend along tail. Therefore, suggest towards end kept alive ICM gentle re-acceleration.