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. Author manuscript; available in PMC: 2018 Apr 20.
Published in final edited form as: Astrophys J. 2017 Apr 18;839(No 2):80. doi: 10.3847/1538-4357/aa69bf

Figure 4.

Figure 4

Growth of fE as a function of θmax,R ∈ {0, θ} illustrated for six values of R0 between 0.1–0.35 at fixed i for the scenario where the shock is around the companion. The curves terminate at θ, resulting in a maximum fE < 0.5 for a prescribed R0 and i. The flat portions at low θmax,R for i = 85° and 90° are due to the companion of R* ≈ 0:1 eclipsing the MSP. Radio observations from Ryba & Taylor (1991) are illustrated with the horizontal dashed lines. Interpretations are discussed in the text.