collaborators

5 papers

astro-ph.HE2026

The Apparent Asymmetric Outflows of TeV Particles from Pulsar Winds

HongYu Pu, Siming Liu

Observations of X-ray filaments attached to a couple of powerful pulsars suggest escape of TeV electrons and/or positrons (e) from pulsar bow shocks into surrounding large…

astro-ph.HE2025

Discovery of diffuse gamma-ray emission in the vicinity of G172.8+1.5: An old supernova remnant with different turbulence properties

Yuan Li, Gwenael Giacinti, Siming Liu

We report the detection of high-energy -ray emission in the vicinity of G172.8+1.5, which is debated as a Supernova remnant (SNR) or an ionized hydrogen (H) region.…

astro-ph.HE2025

Discovery of diffuse -ray emission in the vicinity of G213.0-0.6: Supernova remnant versus massive star-forming region

Yuan Li, Gwenael Giacinti, Siming Liu

We report the discovery of high-energy -ray emission in the vicinity of G213.0-0.6, which is debated as a supernova remnant (SNR) or an ionized hydrogen (H) region.…

astro-ph.HE2025

Influence of interstellar environment near the solar system on cosmic-ray spectra and dipole anisotropy

Zhangxi Xue, Siming Liu

Properties of interstellar environment near the solar system have been probed by missions like IBEX, Voyager over the last two decades. Although it has been well recognized that pr…

astro-ph.HE2025

-Cygni supernova remnant in -rays: signatures of trapped and escaped Cosmic Rays

Yuan Li, Gwenael Giacinti, Siming Liu +1

We reanalyze 15 years of data recorded by the Fermi Large Area Telescope in a region around supernova remnant (SNR) -Cygni from 100 MeV to 1 TeV, and find that the spectra of t…