The bremsstrahlung component of the diffuse galactic gamma-ray emission at MeV-energies

Details The bremsstrahlung component of the diffuse galactic gamma-ray emission at MeV-energies The bremsstrahlung component of the diffuse galactic gamma-ray emission at MeV-energies

Aug 1983

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1983icrc....1..161s&link_type=abstract

IN: International Cosmic Ray Conference, 18th, Bangalore, India, August 22-September 3, 1983, Conference Papers. Volume 1 (A85-2

Physics

Bremsstrahlung, Galactic Cosmic Rays, Gamma Rays, Diffuse Radiation, Energy Spectra, High Energy Electrons

Scientific paper

Recently the galactic plane has been observed at low and medium gamma ray energies in the directions towards the center and anticenter. Spectral measurements are now available at those energies, where the contribution from pion-decay can be neglected. Under the assumption that most of the observed flux below 30 MeV is produced by electron bremsstrahlung, the energy spectrum of cosmic ray electrons in interstellar space below 100 MeV is derived.

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