Ultra-high-energy γ-ray emission associated with the tail of a bow-shock pulsar wind nebula

In this study, we present a comprehensive analysis of an unidentified point-like ultra-high-energy (UHE) γ-ray source, designated as 1LHAASO J1740+0948u, situated in the vicinity of the middle-aged pulsar PSR J1740+1000. The detection significance reached 17.1 σ (9.4 σ) above 25 TeV (100 TeV). The s...

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Bibliographic Details
Format: Article
Language:English
Published: Elsevier 2025-04-01
Series:The Innovation
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Online Access:http://www.sciencedirect.com/science/article/pii/S2666675825000050
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