Cambridge University Press (CUP), Proceedings of the International Astronomical Union, 14(2), p. 374-375, 2006
DOI: 10.1017/s1743921307011052
Full text: Unavailable
AbstractThe 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.