NASA NTRS · 19770014050
Small scale local gamma ray features
Abstract
In order to draw implications from nearby gamma-ray emission, the different ways that can be used to obtain an estimate of the amount of matter on each line of sight are investigated. It is shown that, within present uncertainties, the cosmic ray intensity inside molecular clouds within 1 kpc from the sun is the same as the cosmic ray intensity measured at the sun. In the last part, what can be learned from a comparison of far infrared and gamma-ray data is discussed.
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Puget, J. L., Ryter, C., Serra, G.. 1977-01-01. Small scale local gamma ray features. https://ntrs.nasa.gov/citations/19770014050
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