A brief overview of the PWNe detected by LHAASO

Xi, Shaoqiang

Pulsar wind nebulae (PWNe), powered by the pulsar's rotational energy through the formation and termination of a relativistic electron-positron wind, are bright sources of gamma-rays. The majority of sources detected by LHAASO belong to this population. Here, we offer a brief overview of the PWNe detected by LHAASO and discuss some theoretical implications based on LHAASO observations.