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A search for cosmic-ray acceleration by supernova remnant shocks

โœ Scribed by Osborne, J L; Wolfendale, A W; Zhang, L


Book ID
118160302
Publisher
Institute of Physics
Year
1995
Tongue
English
Weight
411 KB
Volume
21
Category
Article
ISSN
0954-3899

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The discovery using ASCA that the featureless X-ray spectrum from the shell of SN 1006 is produced by shock-accelerated TeV electrons, and is thus an indicator of cosmic ray acceleration, has sparked a search for X-ray spectral evidence for cosmic ray acceleration in other remnants, as well as much