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Publikováno v:
Journal of Physics: Conference Series. 2156:012090
The origin of the gamma-ray halo around pulsars is associated with the reduced diffusivity of energetic particles responsible for gamma-ray emission with respect to the mean-free path they adopt in the interstellar medium. A possible explanation for
Externí odkaz:
https://explore.openaire.eu/search/publication?articleId=doi_________::fdd964f0f302c9bf7d91d061c3148d6a
https://doi.org/10.1088/1742-6596/2156/1/012090
https://doi.org/10.1088/1742-6596/2156/1/012090
