γ Rays from the cosmic ray irradiation of local molecular clouds View Full Text


Ontology type: schema:ScholarlyArticle     


Article Info

DATE

1981-07

AUTHORS

M. R. Issa, A. W. Wolfendale

ABSTRACT

An analysis is given here of the flux of cosmic γ rays of energy above 100 MeV from the directions of 13 local molecular clouds. We show that only in a few clouds does the cosmic ray intensity need to exceed the value near the Earth to explain the γ-ray fluxes. Possible reasons for the few excesses are considered. Our conclusion is important because some of the enigmatic γ-ray ‘sources’ are identified; furthermore, γ-ray data can be coupled with knowledge about the distribution of gas in the Galaxy to throw light on the problem ‘where do cosmic rays come from?’. More... »

PAGES

430-433

References to SciGraph publications

Journal

TITLE

Nature

ISSUE

5822

VOLUME

292

Identifiers

URI

http://scigraph.springernature.com/pub.10.1038/292430a0

DOI

http://dx.doi.org/10.1038/292430a0

DIMENSIONS

https://app.dimensions.ai/details/publication/pub.1012488875


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