Fig. 5.
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HR diagram of 10 402 nearby g-mode pulsators classified as SPB or γ Dor star with a relative parallax uncertainty of better than 3%. The red line is the SPB instability strip from Burssens et al. (2020, at hot temperatures) and the γ Dor instability strip from Dupret et al. (2005, at low temperatures), both for solar metallicity.
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