Acceleration of cosmic rays and gamma-ray emission from supernova remnant/molecular cloud associations
1 APC, Univ. Paris Diderot, CNRS/IN2P3, CEA/Irfu, Obs. de Paris, Sorbonne Paris Cité, France
2 INFN – Gran Sasso Science Institute, viale F. Crispi 7, 67100 L'Aquila, Italy
3 Racah Institute of Physics, The Hebrew University of Jerusalem, 91904, Israel
a Corresponding author: firstname.lastname@example.org
Published online: 8 December 2015
The gamma-ray observations of molecular clouds associated with supernova remnants are considered one of the most promising ways to search for a solution of the problem of cosmic ray origin. Here we briefly review the status of the field, with particular emphasis on the theoretical and phenomenological aspects of the problem.
© Owned by the authors, published by EDP Sciences, 2015
This is an Open Access article distributed under the terms of the Creative Commons Attribution License 4.0, which permits unrestricted use, distribution, and reproduction in any medium, provided the original work is properly cited.