未完成
发表于 2025-3-25 03:20:52
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脱水
发表于 2025-3-25 11:19:20
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tolerance
发表于 2025-3-25 13:43:19
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Confound
发表于 2025-3-25 16:19:06
https://doi.org/10.1007/978-3-030-33124-5The Origin of Cosmic Rays; Galactic Cosmic-Ray Pevatrons; Supernova Remnants; The Galactic Center regio
Anterior
发表于 2025-3-25 20:19:45
2190-5053 and numerical simulations, which are formulated and presented in a straightforward format that can be readily used in the interpretations of gamma-ray and neutrino observations, as well as for confident predictions for future measurements.978-3-030-33126-9978-3-030-33124-5Series ISSN 2190-5053 Series E-ISSN 2190-5061
obligation
发表于 2025-3-26 01:37:15
Gamma-ray and Neutrino Signatures of Galactic Cosmic-ray Accelerators
动脉
发表于 2025-3-26 07:08:19
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META
发表于 2025-3-26 10:10:06
Propagation and Radiation of Accelerated Particles in Supernova Remnants with Clumpy Structures,nerally done on a case by case basis. The case of RX J1713.7-3946 is of special interest in this respect. This remnant has been considered for long time the best candidate for an efficient acceleration scenario, mainly due to its high gamma-ray flux. The detection of gamma-ray emission in the energy
paradigm
发表于 2025-3-26 13:06:40
The Galactic Center Region,ee for an extensive review). It is now in a state of relative inactivity but it might well be a non-stationary source. For instance, there are interesting hints of a much stronger emission few hundreds years ago ; on the timescale of . years, major variability episodes are expected
单片眼镜
发表于 2025-3-26 19:03:03
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