Fig. 10.
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Hertzprung-Russel diagram for the B5 to F-type stars using parameters from Patrick et al. (2025), with stellar evolution tracks from Schootemeijer et al. (2019) labelled according to their initial mass. The filled symbols represent sources whose v sin i measurement is greater than the lower limit of 33 km s−1 by at least 3σ. There is some small overlap with the cool side of Fig. 7.
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