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Particle re-acceleration in the ICM and low-frequency observations

Published online by Cambridge University Press:  01 August 2006

Gianfranco Brunetti
Gianfranco Brunetti*
Affiliation:
INAF – Istituto di Radioastronomia, via P. Gobetti 101, I-40129 Bologna, Italy email: brunetti@ira.inaf.it
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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.

Keywords

acceleration of particlesturbulencegalaxies: clusters: general
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

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