Fig. 20

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Ratio (ν∞/νesc) as a function of temperature. The yellow dashed line is the relation presented in Krtička et al. (2021). The filled red lines represent the ratios from Lamers et al. (1995). The green filled line is the average relation for stars of spectral type earlier than B1 from Hawcroft et al. (2024). The colour gradient correlates to the value of Γe.
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