TeV Gamma Rays and Neutrinos from Winds Driven by Radiatively Inefficient Accretion Flows of Low-Luminosity Active Galactic Nuclei

arXiv:2608.30596 · astro-ph.HE, astro-ph.GA · Submitted 2026-08-31 · Read on arXiv

astro-ph.HE, astro-ph.GA

Submitted: 2026-08-31

Updated: 2026-08-31

Terminology

• AGN — 16× in this paper · explained in 1 episode
• Benchmark — 6× in this paper · explained in 2 episodes
• Accretion Flows — 3× in this paper · explained in 1 episode
• Adam — 3× in this paper · explained in 2 episodes
• Core — 1× in this paper · explained in 2 episodes
• Large High Altitude Air Shower Observatory — 1× in this paper
• National Aeronautics and Space Administration — 1× in this paper
• Very Large Array — 1× in this paper

Sources

• MAGIC observations of NGC 4278. The first low-luminosity radio galaxy with compact jets detected at TeV energies
• Fermi Large Area Telescope Fourth Source Catalog Data Release 4 (4FGL-DR4)
• The Large High Altitude Air Shower Observatory (LHAASO) Science Book (2021 Edition)
• High-energy neutrinos and gamma rays from winds and tori in active galactic nuclei
• Revisiting Disk Winds in Active Galactic Nuclei as an Origin of Cosmic Gamma-ray and Neutrino Backgrounds

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