A cut-off in the TeV gamma-ray spectrum of the SNR Cassiopeia A
Abstract It is widely believed that the bulk of the Galactic cosmic rays is accelerated in supernova remnants (SNRs). However, no observational evidence of the presence of particles of PeV energies in SNRs has yet been found. The young historical SNR Cassiopeia A (Cas A) appears as one of the best c...
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| Published in: | Monthly notices of the Royal Astronomical Society Vol. 472; no. 3; pp. 2956 - 2962 |
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| Main Authors: | , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , , |
| Format: | Journal Article |
| Language: | English |
| Published: |
Oxford University Press
11.12.2017
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| Subjects: | |
| ISSN: | 0035-8711, 1365-2966 |
| Online Access: | Get full text |
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