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Interaction of escaping cosmic rays with molecular clouds

Published online by Cambridge University Press:  29 January 2014

Stefano Gabici
Stefano Gabici*
Affiliation:
APC, AstroParticule et Cosmologie, Université Paris Diderot, CNRS, CEA, Observatoire de Paris, Sorbonne Paris Cité, France – email: stefano.gabici@apc.univ-paris7.fr
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Abstract

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The study of the gamma–ray radiation produced by cosmic rays that escape their accelerators is of paramount importance for (at least) two reasons: first, the detection of those gamma–ray photons can serve to identify the sources of cosmic rays and, second, the characteristics of that radiation give us constraints on the way in which cosmic rays propagate in the interstellar medium. This paper reviews the present status of the field.

Keywords

cosmic rayssupernova remnantsISM: clouds
Type
Contributed Papers
Information
Proceedings of the International Astronomical Union , Volume 9 , Symposium S296: Supernova Environmental Impacts , January 2013 , pp. 320 - 327
Copyright
Copyright © International Astronomical Union 2014 

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