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Fig. 6


Emission maps of the shocked pulsar wind at various frequencies (top to bottom) and for orbital phases φ corresponding to the conjunctions (left and right columns). The emission is displayed on a logarithmic scale ranging from 1 down to 10-4, with 1 corresponding to the maximum value of the emission along the orbit at this frequency (i.e. each map is normalised to its maximum value over any pixel and any φ). The VHE maps do not take the pair production opacity into account. The case shown here corresponds to i = 25° in Fig. 8. The spatial scale is in units of the orbital separation d. See Figs. A.1A.4 for associated movies of the evolution with orbital phase.

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