Red Giant Rotational Inversion Kernels Need Nonlinear Surface Corrections

Asteroseismology is our only means of measuring the rotations of stars in their interiors, rather than at their surfaces. Some techniques for measurements of this kind—“rotational inversions”—require the shapes of linear response kernels computed from reference stellar models to be representative of...

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Bibliographic Details

Published in:	The Astrophysical Journal
Main Author:	J. M. Joel Ong
Format:	Article
Language:	English
Published:	IOP Publishing 2023-01-01
Subjects:	Asteroseismology Perturbation methods Stellar oscillations Stellar rotation Red giant stars
Online Access:	https://doi.org/10.3847/1538-4357/ad0cac