Fig. 16

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Panel A: Comparison between derived terminal velocities (v∞) by this study and those from Hawcroft et al. (2024, small blue diamonds) and Parsons et al. (2024, green squares). The fuchsia hexagons are data from Evans et al. (2004a), which also obtained wind properties via optical and UV analysis with CMFGEN. Panel B: Comparison of the wind microturbulent velocities (ξmax) between this work and Hawcroft et al. (2024). Panel C: Comparison between the sum of v∞ and ξmax, which would roughly translate the width of the absorption component of the UV P Cygni profiles. Panel D: Comparison of the Γ-corrected escape velocities (vesc,Γ) between this study and Hawcroft et al. (2024).
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