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Fig. 5

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Case of the 1.0 M simulations: Log-log of the pulsation period [days] versus the stellar radius, R[R]. We compare the analytical law established here (dashed red curve) with the law from Vassiliadis & Wood (1993) (black curve) and with the fundamental mode from Trabucchi et al. (2019) (dashed black curve). Overall, we found similar trends, only separated by an offset. The pulsation periods of the simulations are shorter than expected.

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