3 papers
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.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
Diagnosing the particle transport mechanism in the pulsar halo via X-ray observations
Qi-Zuo Wu, Chao-Ming Li, Xuan-Han Liang +2
Pulsar halos (also termed 'TeV halo') are a new class of -ray sources in Galaxy, which manifest as extended -ray emission around middle-age pulsars, as discovered around the…