activity
20232025
most citedUltrahigh-Energy Gamma-ray Emission Associated with Black Hole-Jet Systems

9 citations · 13 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.HE2025

Diagnosing the AGN population origin of TeV neutrinos with their spatial correlation

Xiao-Bin Chen, Ruo-Yu Liu, Xiang-Yu Wang

The recent detection of TeV neutrinos from nearby Seyfert galaxies (e.g., NGC 1068) by IceCube suggests that active galactic nuclei (AGNs) could make a significant contribution to…

astro-ph.HE2025

On the origin of ~ 100 TeV neutrinos from the Seyfert galaxy NGC 7469

Qi-Rui Yang, Xiao-Bin Chen, Ruo-Yu Liu +2

The origin of TeV-PeV neutrinos detected by IceCube remains largely unknown. The most significant individual neutrino source is the close-by Seyfert galaxy NGC 1068 at 4.2 level…

astro-ph.HE2025

Potential Contribution of Young Pulsar Wind Nebulae to Galactic High-Energy Neutrino Emission

Xuan-Han Liang, Xiao-Bin Chen, Ben Li +2

Pulsar wind nebulae (PWNe), especially the young ones, are among the most energetic astrophysical sources in the Galaxy. It is usually believed that the spin-down energy injected f…

astro-ph.HE2025★ 1 cited

Detection of a new GeV source in the outer region of the Coma cluster: a signature of external accretion shock ?

Xiao-Bin Chen, Kai Wang, Yi-Yun Huang +4

The supersonic flow motions associated with infall of baryonic gas toward sheets and filaments, as well as cluster mergers, produces large-scale shock waves. The shocks associated…

astro-ph.HE2024

Modeling the X-ray emission of the Boomerang nebula and implication for its potential ultrahigh-energy gamma-ray emission

Xiao-Bin Chen, Xuan-Han Liang, Ruo-Yu Liu +1

The Boomerang nebula is a bright radio and X-ray pulsar wind nebula (PWN) powered by an energetic pulsar, PSR~J2229+6114. It is spatially coincident with one of the brightest ultra…

astro-ph.HE2024★ 9 cited

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.HE2023★ 3 cited

Could the TeV emission of starburst galaxies originate from pulsar wind nebulae?

Xiao-Bin Chen, Ruo-Yu Liu, Xiang-Yu Wang +1

While the GeV -ray emission of starburst galaxies (SBG) is commonly thought to arise from hadronic interactions between accelerated cosmic rays and interstellar gas, the origin…