Skip to main content
. 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 10.

Figure 10

A similar suite of axisymmetric computations as that of Figure 2 but for the parallel-wind shock geometry, with different but appropriate choices θmax,R in the rightmost two panels corresponding to shock tail lengths past the companion of R0 and 4R0.