La gamma astronomie |
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Authors: | E Schatzman |
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Institution: | 1. Institut d'Astrophysique, Paris, France
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Abstract: | It is possible to predict the amount of gamma rays which are produced in various astronomical objects = gamma rays due to nuclear reactions, to bremsstrahlung, to cosmic rays, to annihilation of matter and anti-matter. These predictions are compared to the results of the observations with Explorer XI and are used to suggest new experiments. The following experiments are suggested:- (1)
to measure the γ flash associated with Supernovae;
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