\begin{document}$ 10^{7} $\end{document} and \begin{document}$ 10^{9} $\end{document}m around the pulsar, we obtain the energy distribution of electrons. The leptonic γ-ray spectra can be calculated through inverse Compton scattering processes. The leptonic γ-ray can roughly conform to the observation of LHAASO."> Pulsars as candidates of LHAASO sources J2226+6057, J1908+0621, and J1825-1326: The leptonic origin -
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