Fig. 3
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Velocity stratification υ(r) comparison of the best-fit WN4b β = 1 grid model (H19, black connected circles) and the PoWRHD models in this work (red connected circles) of WR1. The υ(r) of the remaining five targets in this work are shown in cyan for comparison. The range of photospheric radii of the PoWRHD models at optical depth τ = 2/3 R2/3 is shaded in grey. The difference in outermost radii between the grid models and the PoWRHD models is due to the former being traditionally modelled up to 1000 R⊙ and the latter up to 50 000 R*.
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