Image Details
Caption: Figure 3.
Frequencies of ℓ = 0 modes as a function of radial order n for a δ Scuti–like star of M = 1.9 M ⊙, Y i = 0.30, and Z i = 0.020 at the age of 526.4 Myr, computed using MESA and GYRE. We implemented a uniform rotation rate of 1.0 day−1 using the traditional approximation available in GYRE. No quadratic frequency dispersion was observed, even in the nonasymptotic regime.
© 2024. The Author(s). Published by the American Astronomical Society.