Affiliation
CEA/DRF/IRFU/SAp & UMR AIM Paris-Saclay
Main category
Natural Sciences (Astrophysics and Astrononmy)
Alternative category
Natural Sciences (Physics)
Abstract
Most of the information we have about the internal rotation of stars comes from modes that are weakly affected by rotation, for instance thanks to rotational splittings.
In contrast, we present here a method (based on the asymptotic theory of Prat et al. 2016, A&A, 587, A110) which allows us to analyze the signature of rotation where its effect is the most important, that is in low-frequency modes that are strongly affected by rotation.
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