Author

Li-Zhuo Bao

Institution: Beijing Planetarium

Observed institutions: Chinese Academy of Sciences, Beijing Planetarium, Institute of High Energy Physics, University of Chinese Academy of Sciences

ORCID: 0000-0001-7462-1481

Observed ORCID: 0000-0001-7462-1481

OpenAlex ID: A5081726064

Slow Diffusion is Necessary to Explain the γ-Ray Pulsar Halos

2022 · Li-Zhuo Bao, Kun Fang, et al. · The Astrophysical Journal · 38

Features of the gamma-ray pulsar halo HESS J 1831 − 098

2022 · Kun Fang, Shao-Qiang Xi, et al. · Physical review. D/Physical review. D. · 13

Method for testing diffusive shock acceleration and diffusion propagation of 1–100 TeV cosmic electrons with multiwavelength observations of the Geminga halo and pulsar wind nebula

2026 · Weikang Gao, Li-Zhuo Bao, et al. · Physical review. D/Physical review. D. · 1

Works count: 3

Citation count: 52

H-index: 2

I10-index: 2