High Energy Cosmic Rays from Young Neutron Stars
1987 ◽
Vol 125
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pp. 554-554
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Cosmic ray spectrum has an intensity enhancement at energy range 1014–16 eV/nuc. Recently Takahasi et al. (1986) called an attention to chemical composition there. Although the data still contain large uncertainties, they argued an overabundance of calcium at high energies (Ca/Fe ≥ 2 above 1014 eV/nucleus) and some enhancements of medium heavy nuclei (C ∼ Ar) instead of no anomalous p, He, and Fe abundances.
2009 ◽
Vol 18
(10)
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pp. 1577-1581
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2005 ◽
Vol 20
(06)
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pp. 419-440
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2005 ◽
Vol 429
(3)
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pp. 755-765
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2006 ◽
Vol 21
(supp01)
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pp. 192-196
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