activity
20242026
collaborators

5 papers

astro-ph.HE2026

Could the interaction of jet and SN ejecta be the cause of X-ray knots observed in a radio galaxy?

Jia-Chun He, Xiao-Na Sun, Hao-Qiang Zhang +4

We investigate the interaction between relativistic jets and supernova (SN) ejecta as a potential origin of X-ray knots in radio galaxies, employing knot A in M 87 as a test case.…

astro-ph.HE2026

Revisiting the Geminga halo at GeV energies with Fermi-LAT data

Yu Meng, Yun-Feng Liang, Ben-Yang Zhu +2

Nearby pulsars within are considered to be possible sources of 10-500 GeV cosmic-ray positron excess measured by PAMELA and AMS-02. A TeV halo around Geminga is…

astro-ph.HE2025

Ultrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

The LHAASO Collaboration, Zhen Cao, Felix Aharonian +315

Black holes (BH), one of the most intriguing objects in the universe, can manifest themselves through electromagnetic radiation initiated by the accretion flow. Some stellar-mass B…

astro-ph.HE2025

A Giant Peanut-shaped Ultra-High-Energy Gamma-Ray Emitter Off the Galactic Plane

Zhen Cao, Felix Aharonian, Yunxiang Bai +312

Ultra-high-energy (UHE), exceeding 100 TeV (10^12 electronvolts), γ-rays manifests extreme particle acceleration in astrophysical sources. Recent observations by γ-ray telescopes…

astro-ph.HE2024

Extended GeV -ray emission around the star forming region of the W3 complex

Qihang Wu, Xiaona Sun, Ruizhi Yang +3

We analyze the GeV -ray emission from the W3 complex using about 14 years of Pass 8 data recorded by the Large Area Telescope (\textit{Fermi}-LAT). We resolve the $…