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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 11.

Figure 11

Eclipse fraction growth rates for the parallel-wind shock geometry, contrasting the isotropic-winds case in Figure 4. The case i = 55° requires R0 > 0.35 for non-zero fE for all θmax,R and is omitted.