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Particle re-acceleration in the ICM and low-frequency observations
Published online by Cambridge University Press: 01 August 2006
Abstract
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The particle reaceleration model is one of the most promising possibilities to explain the Mpc-scale diffuse radio emission detected in a number of galaxy clusters. Ongoing and future radio observations at low frequencies may help in constraining and testing this model.
- Type
- Contributed Papers
- Information
- Proceedings of the International Astronomical Union , Volume 2 , Highlights of Astronomy 14: Highlights of Astronomy , August 2006 , pp. 374 - 375
- Copyright
- Copyright © International Astronomical Union 2007
References
Ensslin, T. A., Biermann, P. L., Kronberg, P. P., & Wu, X-P. 1997, ApJ, 477, 560CrossRefGoogle Scholar