activity
20152026
most citedA Self-Consistent Explanation of TeV Emissions from HESS J1640-465 and HESS J1641-463

11 citations · 11 across the 5 of their papers we have counts for

collaborators

5 papers

astro-ph.HE2026

Energy-dependent extension of the Crab Nebula as a diagnostic of ultrahigh-energy hadronic emission

Fang-Wu Lu, Bo-Tao Zhu, Ji-Yang Ren +1

The energy-dependent apparent extension of the Crab Nebula, inconsistent with leptonic expectations between X-ray and TeV bands, can be naturally accounted for in a spatially resol…

astro-ph.HE2025

Detection of the Extended -ray Emission around TeV source 1LHAASO J0249+6022 with Fermi-LAT

Gong Yunlu, Zhou Liancheng, Xia Qi +3

1LHAASO J0249+6022 is an extended very-high-energy gamma-ray source discovered by the Large High-Altitude Air Shower Observatory. Based on nearly 16.1 years of data from the Fermi…

astro-ph.HE2025

Multiband Nonthermal Radiative Properties of the Pulsar Wind Nebula CTB 87

Gong Yunlu, Zhou Liancheng, Xia Qi +3

The pulsar wind nebula CTB 87 (G74.9+1.2) is one of the sources emitting -rays with energies higher than 10 TeV, as measured by the Very Energetic Radiation Imaging Telescope Ar…

astro-ph.HE2025

Constraining the Cosmic-ray Energy Based on Observations of Nearby Galaxy Clusters by LHAASO

The LHAASO Collaboration, Zhen Cao, F. Aharonian +323

Galaxy clusters act as reservoirs of high-energy cosmic rays (CRs). As CRs propagate through the intracluster medium, they generate diffuse -rays detectable by arrays such as LH…

astro-ph.HE2015★ 11 cited

A Self-Consistent Explanation of TeV Emissions from HESS J1640-465 and HESS J1641-463

Y. Y. Tang, C. Y. Yang, L. Zhang +1

The bright TeV source HESS J1640-465 is positionally coincident with the young SNR G338.3-0.0, and the nearby HESS J1641-463 with TeV gamma-ray emission seems to be closely associa…