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The cores of active galactic nuclei (AGNs) have been suggested as the sources of IceCube neutrinos, and recent numerical simulations have indicated that hot AGN coronae of Seyfert galaxies and radiatively inefficient accretion flows (RIAFs) of low-luminosity AGNs (LLAGNs) may be promising sites of ion acceleration.
S. Garrappa et al. (Fermi-LAT, ASAS-SN, IceCube), (2019), arXiv:1901.10806 [astro-ph.HE]
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