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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 7.

Figure 7

Orbitally-modulated synchrotron flux ratios of superior-to-inferior conjunction for βmax = {0.5, 0.9} with θmax,X = π/2, at an arbitrary energy where the power-law approximation is valid, for different inclinations and shock stand-off R0 generally consistent with radio eclipses. Phase zero defines SC of the pulsar. The solid and dashed curves are cases, where the shock is shadowed and unshadowed by the companion, respectively.