G. Mou

most citedUltra-high-energy

γ

-ray emission associated with the tail of a bow-shock pulsar wind nebula

3 citations · 3 across the 3 of their papers we have counts for

collaborators

3 papers

astro-ph.HE2025★ 3 cited

Ultra-high-energy $γ$ -ray emission associated with the tail of a bow-shock pulsar wind nebula

Zhen Cao, F. Aharonian, Y. X. Bai +292

In this study, we present a comprehensive analysis of an unidentified point-like ultra-high-energy (UHE) $γ$ -ray source, designated as 1LHAASO J1740+0948u, situated in the vicinity…

astro-ph.HE2025

Broadband $γ$ -ray spectrum of supernova remnant Cassiopeia A

Zhen Cao, F. Aharonian, Y. X. Bai +311

The core-collapse supernova remnant (SNR) Cassiopeia A (Cas A) is one of the brightest galactic radio sources with an angular radius of $\sim$ 2.5 $\arcmin$. Although no extension…

astro-ph.HE2022

An Asymmetrical Model for High Energy Radiation of Cassiopeia A

Shihong Zhan, Wei Wang, Guobin Mou +1

Cassiopeia A (Cas A) supernova remnant shows strong radiation from radio to gamma-ray bands. The mechanism of gamma-ray radiation in Cas A and its possible contribution to PeV cosm…

Ultra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula

Broadband γ-ray spectrum of supernova remnant Cassiopeia A

An Asymmetrical Model for High Energy Radiation of Cassiopeia A

Ultra-high-energy $γ$ -ray emission associated with the tail of a bow-shock pulsar wind nebula

Broadband $γ$ -ray spectrum of supernova remnant Cassiopeia A