High energy galactic gamma radiation from cosmic rays concentrated in spiral arms

Details High energy galactic gamma radiation from cosmic rays concentrated in spiral arms High energy galactic gamma radiation from cosmic rays concentrated in spiral arms

Dec 1974

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1974sfp...........b&link_type=abstract

Submitted for publication

Computer Science

Cosmic Rays, Galactic Radiation, Gamma Rays, Disks (Shapes), Models, Sas-2, Spiral Galaxies

Scientific paper

A model for the emission of high energy ( 100 MeV) gamma rays from the galactic disk was developed and compared to recent SAS-2 observations. In the calculation, it is assumed that (1) the high energy galactic gamma rays result primarily from the interaction of cosmic rays with galactic matter; (2) on the basis of theoretical and experimental arguments the cosmic ray density is proportional to the matter density on the scale of galactic arms; and (3) the matter in the galaxy, atomic and molecular, is distributed in a spiral pattern consistent with density wave theory and the experimental data on the matter distribution.

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