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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 15.

Figure 15

Parallel-wind shock geometry synchrotron light curves contrasting those in Figure 7. Note the different value of R0 for i = 65° required for consistency with radio eclipses.