Titlebook: Galactic Astrophysics and Gamma-Ray Astronomy; Proceedings of a Mee G. E. Morfill,R. Buccheri Conference proceedings 1983 D. Reidel Publish

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Gamma Rays from Close Binary Systems,little interest for explaining the γ-ray sources discovered by the COS-B satellite. Accretion models where there is a non thermal component in the particle energy distribution may be relevant to γ-ray astronomy.

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A Search for Counterparts of Selected Cos-B Galactic Gamma-Ray Sources: The X-Ray Survey and Opticang targets for the HRI instrument capable of an accuracy of ~ 3 arc sec..Due to the misfortunes which occurred to the Einstein satellite, this time-consuming process was feasible only in two cases: within the error circle of 2CG 135 + 01, the radio variable star LSI61.303 was pinpointed by the HRI,

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Large-Scale Structure of the Galaxy and High-Energy Gamma-Ray Observations,d the gas is indicated by the gamma-ray data. The systematic variation with longitude of the spectrum of the gamma-ray emission points to an increased flux of cosmic-ray electrons in the 100 MeV to 1 GeV energy range in regions where dense clouds are concentrated. The variation could as well be due

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peration for another 5 to 10 years, and therefore it is hoped that the proceeding of this meeting can be used (in the intermediate time) as a basis for further studies, as a stimulation for more theoretical work and as an important contribution for defining the aims and operation of future gamma-ray missions.978-94-009-7210-0978-94-009-7208-7

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