商议
发表于 2025-3-25 03:56:26
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加强防卫
发表于 2025-3-25 10:28:24
Book 1976en dent observations (ca. 1975). The high energy ‘Y-rays (>30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail able in this field, even though early t
Colonnade
发表于 2025-3-25 15:36:04
d by indepen dent observations (ca. 1975). The high energy ‘Y-rays (>30MeV) from the Galactic Center are at least partly due to the decay of 1[0 mesons, which are of unique energy (67. 5 MeV) in the 1[0 rest frame only. The reasons for the limited amount of data avail able in this field, even though early t978-90-277-0696-6978-94-010-1496-0
可憎
发表于 2025-3-25 17:18:39
,Theoretical Estimates of γ-Ray Emission,since the results are generally applicable to any astrophysical source where a solar abundance is a reasonable approximation. Only those theoretical predictions for other sources will be discussed here that seem most pertinent to γ-ray line astronomy. The experimental evidence for γ-ray fluxes in th
废止
发表于 2025-3-25 21:39:02
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flex336
发表于 2025-3-26 03:32:57
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Noctambulant
发表于 2025-3-26 04:51:34
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肉体
发表于 2025-3-26 09:52:41
Introduction,raph we discuss only the three decades of energy from ~10.eV to 10.eV, where nuclear γ-ray lines are expected. The most recent comprehensive review of the general fields of X-ray and γ-ray astronomy has been given by Greisen (1971) and this should be consulted for a broad perspective of the astrophy
hysterectomy
发表于 2025-3-26 15:14:09
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Madrigal
发表于 2025-3-26 19:36:52
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