Asteroseismology and Interferometry
M. S. Cunha, C. Aerts, J. Christensen-Dalsgaard, A. Baglin, L. Bigot,, T. M. Brown, C. Catala, O. L. Creevey, A. Domiciano de Souza, P. Eggenberger,, P. J. V. Garcia, F. Grundahl, P. Kervella, D. W. Kurtz, P. Mathias, A., Miglio, M. J. P. F. G. Monteiro, G. Perrin, F. P. Pijpers

TL;DR
This paper reviews how asteroseismology and interferometry together enhance understanding of stellar structures, discusses current limitations, and explores future observational prospects and technological developments in the field.
Contribution
It provides a comprehensive review of the integration of asteroseismology and interferometry, highlighting recent studies, limitations, and future instrument developments.
Findings
Recent pilot studies combining asteroseismic and interferometric data.
Identification of current limitations in mode detection and parameter measurement.
Discussion of future instruments and satellite missions for improved observations.
Abstract
Asteroseismology provides us with a unique opportunity to improve our understanding of stellar structure and evolution. Recent developments, including the first systematic studies of solar-like pulsators, have boosted the impact of this field of research within Astrophysics and have led to a significant increase in the size of the research community. In the present paper we start by reviewing the basic observational and theoretical properties of classical and solar-like pulsators and present results from some of the most recent and outstanding studies of these stars. We centre our review on those classes of pulsators for which interferometric studies are expected to provide a significant input. We discuss current limitations to asteroseismic studies, including difficulties in mode identification and in the accurate determination of global parameters of pulsating stars, and, after a…
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