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Chao-Ming Li

4 papers hereh-index 17 citations4 works total

Matching runs newest-first, so older work may not be attached to this profile yet.

author position
  • first author2
  • middle author2

Across the 4 of 4 papers where every author was matched, so the position is known.

fields
  • astro-ph.HE4

identity via Semantic Scholar / OpenAlex

most citedDiagnosing Interstellar Magnetic Turbulence with TeV Pulsar Halos

1 citations · 1 across the 4 of their papers we have counts for

collaborators

4 papers

astro-ph.HE2026

Galactic Cosmic Ray Transport in the Giant Circumgalactic Medium Halo

Chao-Ming Li, Andrew M. Taylor

Recent observations have revealed that the Milky Way is embedded in a massive circumgalactic medium (CGM) extending to several hundred kiloparsecs. Such an extended gaseous halo ac…

astro-ph.HE2026

Anisotropic Diffusion in Pulsar Halos: Interpreting the asymmetric morphology of Geminga and Monogem halos measured by HAWC

Si-Zhe Wu, Chao-Ming Li, Ruo-Yu Liu

Pulsar halos are produced by electrons and positrons diffusing in the interstellar medium around their parent pulsar wind nebulae. Recent observations by HAWC and LHAASO have revea…

astro-ph.HE2026★ 1 cited

Diagnosing Interstellar Magnetic Turbulence with TeV Pulsar Halos

Chao-Ming Li, Ruo-Yu Liu, Huirong Yan

Interstellar magnetic field is essential in various astrophysical phenomena and processes. Pulsar halos are a recently discovered class of TeV gamma-ray sources formed by escaping…

astro-ph.HE2024

Diagnosing the particle transport mechanism in the pulsar halo via X-ray observations

Qi-Zuo Wu, Chao-Ming Li, Xuan-Han Liang +2

Pulsar halos (also termed 'TeV halo') are a new class of γ-ray sources in Galaxy, which manifest as extended γ-ray emission around middle-age pulsars, as discovered around the…

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Not affiliated with arXiv. Researcher data from Semantic Scholar (ODC-BY) and OpenAlex.