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发表于 2025-2-13 15:39:48
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摘要(1):Gamma-ray observations provide important information on cosmic-ray (CR) propagation in our Galaxy. First, we discuss TeV halos. We show that current gamma-ray measurements place interesting constraints on the turbulent magnetic fields around these pulsars, and we examine the implications for CR transport. Also, we suggest that extended gamma-ray sources of a hadronic origin should exist in the data. We show that such a source might exist in the AS-gamma data at 398-1000 TeV. Observations of this new type of sources could be used to constrain the Galactic magnetic field geometry. |
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