Excess gamma rays from the Loop I supernova remnant

Details Excess gamma rays from the Loop I supernova remnant Excess gamma rays from the Loop I supernova remnant

Aug 1985

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1985icrc....1..342b&link_type=abstract

In NASA. Goddard Space Flight Center 19th Intern. Cosmic Ray Conf., Vol. 1 p 342-344 (SEE N85-33902 22-93)

Astronomy and Astrophysics

Astronomy

Cosmic Gases, Cosmic Rays, Gamma Rays, Gas Density, North Polar Spur (Astronomy), Radiant Flux Density, Supernova Remnants, Carbon Monoxide, Cos-B Satellite, Hydrogen, Interstellar Matter, Molecular Gases, Sas-2

Scientific paper

Evidence is presented for an excess of cosmic ray intensity within the Loop I supernova remnant, based on an interpretation of the observed distribution of γ-rays across the remnant and the column densities of the associated gas. A strong case can thus be made for the bulk of the cosmic radiation (E < 1011eV) being produced in the Galactic supernova remnants.

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