We aim to obtain a consistent description of non-thermal emissions from Abell 2256 and to give a prediction for a gammaray emission from this galaxy cluster. Assuming that a radio relic illuminates a localization of an ongoing merger, and that both radio and non-thermal part of hard X-ray emission a
Radio emission of galaxy clusters
✍ Scribed by I. Golombek; M. Bartelmann; T. Enßlin; M. Jubelgas; C. Pfrommer; V. Springel
- Publisher
- John Wiley and Sons
- Year
- 2006
- Tongue
- English
- Weight
- 204 KB
- Volume
- 327
- Category
- Article
- ISSN
- 0004-6337
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