Fig. 11

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Comparison between the output mass-loss rates of the T* sequence (red curve) and different recipes applied to the stellar properties of each model. The thick purple and fuchsia lines indicate the mass-loss rates by Vink et al. (2001), applied to T* and T2/3, respectively. The thin lines of the same colors indicate the Vink rates with an offset of 0.8 dex. The yellow curve indicates the rates of Björklund et al. (2023), and the teal line indicates the rates of Krtička et al. (2024), both applied to T2/3. The green line indicates the rates computed using the tool LIME (https://lime.ster.kuleuven.be/, Sundqvist et al. 2025).
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