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Ultra-high-energy g-ray emission associated with the tail of a bowshock pulsar wind nebula
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作者 The LHAASO Collaboration r.x. +4 位作者 K.W. S.C. R.L. S.X. S.H. 《The Innovation》 2025年第4期66-70,65,共6页
In this study,we present a comprehensive analysis of an unidentified pointlike ultra-high-energy(UHE)g-ray source,designated as 1LHAASO J1740+0948u,situated in the vicinity of the middle-aged pulsar PSR J1740+1000.The... In this study,we present a comprehensive analysis of an unidentified pointlike ultra-high-energy(UHE)g-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 s(9.4 s)above 25 TeV(100 TeV). 展开更多
关键词 lhaaso j u detection significance bowshock pulsar wind nebula psr j pointlike source ultra high energy gamma rays middle aged pulsar
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