Fig. 2.
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Hertzsprung-Russell diagrams showing the sample of g-mode pulsators with Ppred ≥ 0.5 (grey symbols with error bars). The evolutionary tracks show the extend of the grid of rotating stellar models, covering a mass range of [1.3, 9] M⊙, where the black (red) colour indicates ω0 = 0.05 (0.55), and the solid (dashed) line style fCBM = 0.005 (0.025).
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