Fig. 2.
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Main-sequence tracks of a M = 1.6 M⊙γ Dor star and a M = 5 M⊙ SPB star in the Hertzsprung–Russell diagram. The crossed (respectively hatched) area roughly indicates the region where γ Dor (respectively SPB) stars are expected to host gravity modes (Aerts et al. 2010, Appendix A). Yellow, blue, and purple stars indicate the chosen models at ZAMS, mid-MS, and TAMS, respectively.
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