The Spiral Structure Interstellar Medium and Cosmic-Rays as Derived from Gamma-Ray Emission of the Galactic Disk

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The gas distribution within the galactic disk accounting for the observed longitudinal distribution of galactic gamma-ray emission Fobs(l) is derived. Unlike the results of other papers interpreting the galactic gamma-ray emission, it is shown that the latter indicates the existence of galactic shocks, and that Fobs(l) may be explained without the hypothesis that cosmic rays are strongly coupled to the gas.

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