NASA NTRS · 19740006371
Galactic gamma rays: Models involving variable cosmic-ray density
Abstract
Mathematical models were developed to determine variable cosmic ray flux around the galactic plane. Data indicate point sources, molecular hydrogen concentration, increased cosmic ray density toward the galactic center, and neutral pion production combine to cause radiation density variables in the galactic plane.
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Strong, A. W., Wdowczyk, J., Wolfendale, A. W.. 1973-01-01. Galactic gamma rays: Models involving variable cosmic-ray density. https://ntrs.nasa.gov/citations/19740006371
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