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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…
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…
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…
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 -ray sources in Galaxy, which manifest as extended -ray emission around middle-age pulsars, as discovered around the…