Fig. 7: Differences in pulsation frequency between the 34 disk-mediated accretion models and the classical models for the input physics with increased envelope mixing. | Nature Communications

Fig. 7: Differences in pulsation frequency between the 34 disk-mediated accretion models and the classical models for the input physics with increased envelope mixing.

From: The imprint of star formation on stellar pulsations

Fig. 7

The violin plots are similar to those shown in the lower panels in Fig. 5. The grey areas mark the Rayleigh limit corresponding to 4 year Kepler (dark grey) and 357 days TESS light curves (light grey). a Results at the pre-main sequence stage. b Results at the ZAMS.

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