Titlebook: Gamma-Ray Astronomy; Nuclear Transition R E. L. Chupp Book 1976 D. Reidel Publishing Company, Dordrecht, Holland 1976 Supernova.astronomy.a

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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

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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

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,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

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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

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