no code implementations • 5 Jan 2021 • Sheng-Hao Wang, Kun Fang, Xiao-Jun Bi, Peng-Fei Yin
The TeV $\gamma$-ray halo around the Geminga pulsar is an important indicator of cosmic-ray (CR) propagation in the local zone of the Galaxy as it reveals the spatial distribution of the electrons and positrons escaping from the pulsar.
High Energy Astrophysical Phenomena High Energy Physics - Phenomenology
