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Fig. 12.
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Terminal velocity vs. Temperature for our sample stripped stars. The position of WR stars in the Magellanic clouds (Shenar et al. 2016, 2019), theoretical WN model sequences (black lines) from Sander et al. (2023), and the correlation for OB stars from the ULLYSES sample (Hawcroft et al. 2024) are shown for comparison.
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