Likely detection of GeV γ-ray emission from pulsar wind nebula G32.64+0.53 with Fermi-LAT

Yifan Xiao(Yunnan University), Jun Fang(Yunnan University), Keyao Wu(Yunnan University)
arXiv (Cornell University)
August 13, 2024
10.48550/arxiv.2408.06939
Cited by 0

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