Speaker
Yu Luo
(Shanghai Jiao Tong University)
Description
A major fraction of gamma-ray sources in the non-thermal universe are pulsar wind nebulae (PWNe), which evolve rapidly and exhibit distinct morphological and spectral features at different evolutionary stages. LHAASO has identified dozens of TeV sources associated with pulsars, which are potential candidates for PWNe or halos. In this study, we use LHAASO data to investigate the relationship between the pulsars and the TeV emissions from their associated nebulae or halos, aiming to better understand the evolution of PWNe.
| Collaboration(s) | LHAASO |
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