Measurements of the low-energy gamma ray continuum emission from the Galactic Center direction

Details Measurements of the low-energy gamma ray continuum emission from the Galactic Center direction Measurements of the low-energy gamma ray continuum emission from the Galactic Center direction

Jul 1982

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1982stin...8312035j&link_type=abstract

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Computer Science

Bremsstrahlung, Continuous Radiation, Galactic Nuclei, Gamma Rays, Low Frequencies, Power Spectra, Relativistic Particles, Balloon-Borne Instruments, Continuum Flow, Galactic Radiation, Gamma Ray Telescopes, Particle Emission, Radiation Measurement

Scientific paper

Using the data obtained with a balloon-borne gamma-ray telescope to measure gamma-rays in the energy interval between 0.3 and 3 MeV, two points for the continuum spectrum in the range between 0.34 and 0.67 MeV were calculated. The power law spectrum suggests that the main component for the gamma-ray continuum emission below 10 MeV is dominated by the bremsstrahlung due to relativistic electrons.

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