Fig. 10
Comparison of the velocity fields in the self-consistent hydrodynamic simulations (solid lines) to fits assuming “single” (dashed lines) and “double” (dashed-dotted lines) β-laws. See text. The dotted background lines compare the fits to simple β = 0.5 and β = 1.0 laws. Upper and lower panels: late and early O-star models from Table 1, respectively.
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