Fig. 1.

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Guitar Nebula: Color map of the ratio, γesc/γMPD (base-10 logarithm, left panel), and the efficiency, ϵ (right panel), as a function of the pulsar velocity, Vpsr (within the estimated uncertainty; de Vries et al. 2022), and the ambient number density, nISM. The black curve shows the relation we used to estimate nISM (pressure equilibrium at the bow shock standoff distance, d0). The black points indicate the position of the system for the best estimate of Vpsr (and nISM).
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