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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: [email protected]
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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

References

Blasi, P. 2004, J. Korean Astron. Soc. 37, 483CrossRefGoogle Scholar
Berezinsky, V. S., Blasi, P., & Ptuskin, V. S. 1997, ApJ, 487, 529CrossRefGoogle Scholar
Brunetti, G. 2006, AN, 327, 615Google Scholar
Brunetti, G., Setti, G., Feretti, L., & Giovannini, G. 2001, MNRAS, 320, 365CrossRefGoogle Scholar
Brunetti, G., Blasi, P., Cassano, R., & Gabici, S. 2004, MNRAS, 350, 1174CrossRefGoogle Scholar
Buote, D. A. 2001, ApJ (Letters), 553, L15CrossRefGoogle Scholar
Cassano, R., & Brunetti, G. 2005, MNRAS, 357, 1313CrossRefGoogle Scholar
Cassano, R., Brunetti, G., & Setti, G. 2006, MNRAS, 369, 1577CrossRefGoogle Scholar
Dolag, K. 2006, AN, 327, 575Google Scholar
Ensslin, T. A., Biermann, P. L., Kronberg, P. P., & Wu, X-P. 1997, ApJ, 477, 560CrossRefGoogle Scholar
Feretti, L. 2005, Adv. Space Res., 36, 729CrossRefGoogle Scholar
Giovannini, G., Tordi, M., & Feretti, L. 1999, New Astron., 4, 141CrossRefGoogle Scholar
Hwang, C.-Y. 2004, J. Korean Astron. Soc., 37, 461CrossRefGoogle Scholar
Jaffe, W. J. 1977, ApJ, 212, 1CrossRefGoogle Scholar
Petrosian, V. 2001, ApJ, 557, 560CrossRefGoogle Scholar
Sarazin, C. 2004, J. Korean Astron. Soc., 37, 433CrossRefGoogle Scholar
Subramanian, K., Shukurov, A., & Haugen, N. E. L. 2006, MNRAS, 366, 1437CrossRefGoogle Scholar
Venturi, T., Parma, P., de Ruiter, H. R. 2006, MemSAI Suppl., 10, 111Google Scholar
Venturi, T., Giacintucci, S., Brunetti, , et al. 2007, A&A, 463, 937Google Scholar
Völk, H. J., Aharonian, F. A., & Breitschwerdt, D. 1996, Space Sci. Revs., 75, 279Google Scholar