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Young Stars Emit More High-Energy Radiation


Book ID
124681356
Publisher
JSTOR
Year
1963
Weight
347 KB
Volume
84
Category
Article
ISSN
0096-4018

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Young, rapidly rotating neutron stars could accelerate protons to energies of โˆผ 1 PeV close to the stellar surface, which scatter with x-rays from the stellar surface through the ฮ” resonance and produce pions. The pions subsequently decay to produce muon neutrinos. We find that the energy spectrum o