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Constraints on the magnetic field in the hadronic scenario for the origin of the radio halo in the A1795 galaxy cluster
The radio halo in the cool-core galaxy cluster, A1795, has recently been proposed to be of hadronic origin, because it extends on megaparsec scales, where no turbulence is expected to be injected into a relaxed cluster. In this paper we aim to constrain the properties of nonthermal protons and the c
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