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3HWC J0631+107/LHAASO J0631+1040: a TeV halo powered by the pulsar J0631+1036?
Dong Zheng, Zhongxiang Wang, Yi Xing
PSR~J0631+1036 is a middle-aged pulsar with properties similar to those of the nearby Geminga pulsar. It is bright in -rays, and has been noted as the only source possibly assoc…
Two Candidate Pulsar TeV Halos Identified from Property-Similarity Studies
Dong Zheng, Zhongxiang Wang
TeV halos have been suggested as a common phenomenon associated with middle-aged pulsars. Based on our recent work on PSR~J0631+1036, which is the only known source positionally co…
4FGL J1844.4-0306: high-energy emission likely from the supernova remnant G29.37+0.1
D. Zheng, Z. Wang, X. Zhang +2
Very-high-energy (VHE) observations have revealed approximately 100 TeV sources in our Galaxy, and a significant fraction of them are under investigation for understanding their or…
On the Gamma-Ray Emission of the Andromeda Galaxy M31
Yi Xing, Zhongxiang Wang, Dong Zheng +1
Using the -ray data obtained with the Large Area Telescope (LAT) onboard {\it the Fermi Gamma-ray Space Telescope (Fermi)} for 14 years, we examine the high energy emissio…