17 citations · 59 across the 5 of their papers we have counts for
9 papers
High-energy studies of the 3HWC J1954+286 region: likely Gamma-ray detection of the supernova remnant G65.1+0.6
Y. Xing, D. Zheng, Z. Wang +3
We carry out high-energy studies of the region of the Galactic TeV source 3HWC J1954+286, whose location coincides with those of PSR~J1954+2836 and supernova remnant (SNR) G65.1+0.…
Modeling the broadest spectral band of the Crab nebula and constraining the ions acceleration efficiency
Xiao Zhang, Yang Chen, Jing Huang +1
Although it is widely accepted that the electromagnetic spectrum from radio to very-high-energy -rays of pulsar wind nebulae (PWNe) originates from leptons, there is still an op…
A Small-Scale Investigation of Molecular Emission toward the Tip of the Western Lobe of W50/SS433
Qian-Cheng Liu, Yang Chen, Ping Zhou +2
We perform a molecular (CO and CN) line observation using IRAM 30m telescope toward two small regions near the western edge of supernova remnant (SNR) W50/SS433. CO observation rev…
Electron Acceleration in Middle-age Shell-type -Ray Supernova Remnants
Xiao Zhang, Siming Liu
Over the past decade, -ray observations of supernova remnants (SNRs) and accurate cosmic-ray (CR) spectral measurements have significantly advanced our understanding of particle…
Fermi LAT detection of the supernova remnant SN 1006 revisited: the south-west limb
Yi Xing, Zhongxiang Wang, Xiao Zhang +1
The data from the Large Area Telescope (LAT) onboard the Fermi Gamma-ray Space Telescope have recently been updated. We thus re-analyze the LAT data for the supernova remnant (SNR)…
Is Supernova Remnant Cassiopeia A a PeVatron?
Xiao Zhang, Siming Liu
Cassiopeia A, a well-observed young core-collapse supernova remnant (SNR), is considered as one of the best candidates for studying very high-energy particle acceleration up to PeV…