Possible origin of the slow-diffusion region around Geminga
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DOI: 10.1093/mnras/stz1974
Abstract: Geminga pulsar is surrounded by a multiTeV γ-ray halo radiated by the high-energy electrons and positrons accelerated by the central pulsar wind nebula (PWN). The angular profile of the γ-ray emission reported by High-Altitude Water… read more here.
Keywords: geminga; electrons positrons; around geminga; slow diffusion ... See more keywords