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Published in 2020 at "Monthly Notices of the Royal Astronomical Society"
DOI: 10.1093/mnras/staa1807
Abstract: Oscillation mode frequencies of stars are typically treated as static for a given stellar model. However, in reality they can be perturbed by time varying sources such as magnetic fields and flows. We calculate the…
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Keywords:
oscillations magnetic;
sensitivities solar;
like oscillations;
empirical relations ... See more keywords