Primary gamma-rays with E gamma or = to 10(15) eV: Evidence for ultrahigh energy particle acceleration in galactic sources

Details Primary gamma-rays with E gamma or = to 10(15) eV: Evidence for ultrahigh energy particle acceleration in galactic sources Primary gamma-rays with E gamma or = to 10(15) eV: Evidence for ultrahigh energy particle acceleration in galactic sources

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..255a&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 255-258 (SEE N85-33902 22-93)

Physics

Cosmic Ray Showers, Galactic Evolution, Gamma Rays, High Energy Interactions, Background Radiation, Energy Spectra, Spectrum Analysis

Scientific paper

The recently observed primary ultra high energy gamma-rays (UHEGR)
testify to the cosmic ray (CR) acceleration in the Galaxy. The available
data may be interpreted as gamma-ray production due to photomeson
production in CR sources.

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