A Model for Magnetic Reconnection as the Origin of TeV Outbursts from NGC 1275
Zhen-Jie Wang, Hong-Bin Tan, Ruo-Yu Liu
astro-ph.HE
Submitted: 2026-06-26
Comments: 10 pages, 7 figures, accepted for publication in PRD
Journal ref: Phys. Rev. D 114(2026), 043003
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Relativistic Jets in Active Galactic Nuclei
- Broadband multi-wavelength study of LHAASO detected AGN
- Multiple Emission Regions in Jets of Low Luminosity Active Galactic Nucleus in NGC 4278
- Hadronuclear interactions in the jet of low TeV luminosity AGN: Implications for the low-state very-high-energy gamma-ray emission
- Fast TeV variability in blazars: jets in a jet
- Reconnection-driven plasmoids in blazars: fast flares on a slow envelope
- Fast magnetic reconnection in the plasmoid-dominated regime
- Relativistic Magnetic Reconnection in Astrophysical Plasmas: A Powerful Mechanism of Nonthermal Emission
- MAGIC discovery of VHE Emission from the FSRQ PKS 1222+21
- A Tight Connection between Gamma-Ray Outbursts and Parsec-Scale Jet Activity in the Quasar 3C 454.3
- Kinematics and Excitation of the Molecular Hydrogen Accretion Disc in NGC 1275
- A wide and collimated radio jet in 3C 84 on the scale of a few hundred gravitational radii
- Fermi Discovery of Gamma-Ray Emission from NGC 1275
- Detection of very-high energy \gamma-ray emission from NGC 1275 by the MAGIC telescopes
- Contemporaneous observations of the radio galaxy NGC 1275 from radio to very high energy gamma-rays
- A Non-thermal Study of the Brightest Cluster Galaxy NGC 1275 - The Gamma-Radio Connection Over Four Decades
- Detection of two TeV gamma-ray outbursts from NGC 1275 by LHAASO
- Very High-energy Gamma-Ray Episodic Activity of Radio Galaxy NGC 1275 in 2022-2023 Measured with MACE
- Observational Evidence to Support a Dense Ambient Medium Shaping the Jet in 3C 84
- Compton-induced $\gamma$-ray Cascade Emissions in Radio Galaxy NGC 1275
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