Adding a harmonic term at twice the acoustic depth reconciles frequency, second-difference, and ratio measurements of the convective envelope base in F-type stars, aligning them with stellar models.
I., Reiners, A., & Solanki, S
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Glitches in solar-like oscillating F-type stars: Possible contribution of non-linear terms
Adding a harmonic term at twice the acoustic depth reconciles frequency, second-difference, and ratio measurements of the convective envelope base in F-type stars, aligning them with stellar models.