Fig. 14
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sHR diagram of the stars in the sample color-coded by log Q. The bottom and right subpanels in each panel show this quantity against Teff and log ℒ, respectively. Cases in which log Q is degenerate are excluded (see Sect. 4.1). All panels include 191 O-type stars from Hol18-22 (gray circles). The evolutionary tracks are the same as in Fig. 7 for Geneva models.
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