Constraints on the magnetic field in the hadronic scenario for the origin of the radio halo in the A1795 galaxy cluster

arXiv:2607.24397 · astro-ph.HE, astro-ph.CO · Submitted 2026-07-27 · Read on arXiv

astro-ph.HE, astro-ph.CO

Submitted: 2026-07-27

Updated: 2026-08-28

Comments: 5 pages, 1 appendix, 4 figures, 1 table; accepted for publication in A&A

DOI: 10.1051/0004-6361/202661115

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Core — 6× in this paper · explained in 2 episodes
• Adam — 4× in this paper · explained in 2 episodes
• Benchmark — 2× in this paper · explained in 2 episodes
• Degeneracy — 1× in this paper · explained in 3 episodes
• Fermi-Large Area Telescope — 1× in this paper

Sources

• XRISM Observations of Abell 1795: Evidence for Low Turbulence and Resonant Scattering
• Study of Polarized Emission in Radio Halos and Filaments in the SKA Telescopes Era

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