Similar to Figure 3, but with various efficiency and AML modes of the evaporative wind. From top to bottom rows, the evaporative wind is assumed to carry the specific angular momentum of the donor star (Mode A), at the inner Lagrangian point (Mode B), and no AM (Mode C), respectively. The evaporation efficiency is taken to be ﹩f=0.1,﹩ 0.2, and 0.3 for Mode A and 0.04, 0.1, and 0.2 for Modes B and C. Also plotted are black widow systems in the Galactic field (Field BWs) and globular clusters (GC BWs), with blue symbols.