Using a fast approximation for radiative accelerations in stellar models changes predicted surface calcium in F-type stars but barely affects inferred masses, radii, and ages.
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Impact of radiative accelerations on the stellar characterization of FGK-type stars using spectroscopic and seismic constraints
Using a fast approximation for radiative accelerations in stellar models changes predicted surface calcium in F-type stars but barely affects inferred masses, radii, and ages.