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This article has an erratum: [https://doi.org/10.1051/0004-6361/201116530e]


Fig. 8

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Distance, expressed in Mpc, at which the radio emission produced in the companion’s Alfvén wing can reach a flux density of 1 Jy, for various distances from the pulsar to its companion. The values that are not varied are the same as in the text. They correspond to a recycled millisecond pulsar and a coefficient ϵ = 10-3. The radio spectrum is assumed to be spread over a spectral range of 1 GHz.

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