D. Wei

most citedUltra-high-energy

γ

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

3 citations · 3 across the 2 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-ph2005

High Energy Afterglow Emission from Giant Flares of Soft Gamma-Ray Repeaters: The Case of the 2004 December 27 Event from SGR 1806-20

Y. Z. Fan, Bing Zhang, D. M. Wei

We discuss the high enegry afterglow emission (including high energy photons, neutrinos and cosmic rays) following the 2004 December 27 Giant Flare from SGR 1806-20. If the initial…

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

High Energy Afterglow Emission from Giant Flares of Soft Gamma-Ray Repeaters: The Case of the 2004 December 27 Event from SGR 1806-20

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