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
โฆ LIBER โฆ
Cosmic ray acceleration by supernova shocks
โ Scribed by E.G. Berezhko
- Publisher
- Elsevier Science
- Year
- 2008
- Tongue
- English
- Weight
- 380 KB
- Volume
- 41
- Category
- Article
- ISSN
- 0273-1177
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