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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Origin of the Diffuse Galactic Gamma-Ray Emission at Low and Medium Gamma-Ray Energies,al measurements are now available at those energies, where the contribution from π°-decay gamma rays can be neglected. The high MeV-fluxes observed in both parts of the Galaxy are an indication of either a strong electron induced component or a high contribution from unresolved sources. Several inte

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The Use of Gamma Rays to Trace the Local Interstellar Hydrogen, from galaxy counts. It is found that to a good approximation the gamma-ray intensity is proportional to the total gas column density, and on this basis a map of the angular distribution of local molecular hydrogen at intermediate latitudes is presented. Comparing this with a simular map produced fr

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Fatten

Comparison of Far-Infrared Radiation with Gamma Radiation,ow component might result from the interaction between cosmic rays and H. gas. The mass of gas in the Galactic Center is not large enough to produce the gamma-ray peak, but enough to produce the far-infrared peak. The relation of far-infrared dip and near-infrared hump near . = 356° to gamma-ray hum

Antimicrobial

Conference proceedings 1983in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were livel- sometimes heated - and the original time span allocated to the meeting was as a result, comfortably exceeded by about 50 % . The aim of this meeting was to determine the role of galactic gam

連鎖,連串

IAU, held in Patras, August 19, 1982. Roughly one hundred scientists attended this meeting, the discussions were livel- sometimes heated - and the original time span allocated to the meeting was as a result, comfortably exceeded by about 50 % . The aim of this meeting was to determine the role of ga

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