Signatures of Core-envelope Rotational Misalignment in the Mixed-mode Asteroseismology of Kepler-56

Existing asteroseismic rotational measurements assume that stars rotate around a single axis. However, tidal torques from misaligned companions, or their possible engulfment, may bring the rotational axis of a star's envelope out of alignment with its core, breaking azimuthal symmetry. I derive...

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Bibliographic Details
Main Author: J. M. Joel Ong
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Online Access:https://doi.org/10.3847/1538-4357/ada4a3
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