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[en] An examination is made of the contribution to the number of apparently discrete sources of γ-rays from cosmic rays interacting with molecular clouds in the Galaxy. Attention is directed to specific nearby clouds and to clouds in general, the latter by a Monte-Carlo analysis. (author)
Journal
Philosophical Transactions of the Royal Society of London. Series A: Mathematical and Physical Sciences; ISSN 0080-4614; 
; v. 301(1462); p. 533-535
; v. 301(1462); p. 533-535