Observations of medium energy gamma ray emission from the galactic center region

Details Observations of medium energy gamma ray emission from the galactic center region Observations of medium energy gamma ray emission from the galactic center region

Apr 1978

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1978stin...7824032k&link_type=abstract

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Cosmic Rays, Gamma Rays, Milky Way Galaxy, Bremsstrahlung, Spectral Emission, Spectral Energy Distribution, Spectrum Analysis

Scientific paper

Measurements of the gamma-ray emission in the medium energy range between 15 and 100 MeV, obtained during two ballon flights from Brazil are presented. The importance of this energy region in determining whether pi deg - decay of electron bremsstrahlung is the most likely dominant source mechanism is discussed along with the implications of such observations. Specifically, the data from this experiment suggest that emission from the galactic plane is similar to theoretical spectrum calculations including both sources mechanisms, but with the bremsstrahlung component enhanced by a factor of about 2. A spectral distribution of gamma-rays produced in the residual atmosphere above the instrument is also presented and compared with other data. A rather smooth spectral variation from high to low energies is found for the atmospheric spectrum.

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