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• W3143114686 startingPage "127" @default.
• W3143114686 abstract "Observations of the Small Magellanic Cloud using the Energetic Gamma Ray Experiment Telescope on the Compton Observatory yield an upper limit (95% confidence) for gamma-ray emission >100 MeV of 0.5ifmmodetimeselsetexttimesfi{}${10}^{mathrm{ensuremath{-}}7}$ photon/${mathrm{cm}}^{2}$ s. The expected flux if the cosmic rays are universal rather than galactic in origin, is (2.4-0.5)ifmmodetimeselsetexttimesfi{}${10}^{mathrm{ensuremath{-}}7}$ photon/${mathrm{cm}}^{2}$ s, only a third of which arise from cosmic ray electron interactions. Hence, the bulk of the cosmic ray energy density is almost certainly not metagalactic, and therefore galactic in origin." @default.
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• W3143114686 date "1993-01-11" @default.
• W3143114686 modified "2023-09-30" @default.
• W3143114686 title "Constraints on the cosmic rays in the Small Magellanic Cloud" @default.
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• W3143114686 doi "https://doi.org/10.1103/physrevlett.70.127" @default.
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