---
res:
  bibo_abstract:
  - Asteroseismology is the study of the interior physics and structure of stars using
    their pulsations. It is applicable to stars across the Hertzsprung–Russell (HR)
    diagram and a powerful technique not only to measure masses, radii, and ages but
    also directly constrain interior rotation, chemical mixing, and magnetism. This
    is because a star's self-excited pulsation modes are sensitive to its structure.
    Asteroseismology generally requires long-duration and high-precision time-series
    data. The method of forward asteroseismic modeling, which is the statistical comparison
    of observed pulsation mode frequencies to theoretically predicted pulsation frequencies
    calculated from a grid of models, provides precise constraints for calibrating
    various transport phenomena. In this introduction to asteroseismology, we provide
    an overview of its principles, and the typical data sets and methodologies used
    to constrain stellar interiors. Finally, we present key highlights of asteroseismic
    results from across the HR diagram, and conclude with ongoing challenges and future
    prospects for this ever-expanding field within stellar astrophysics.@eng
  bibo_authorlist:
  - foaf_Person:
      foaf_givenName: Dominic M.
      foaf_name: Bowman, Dominic M.
      foaf_surname: Bowman
  - foaf_Person:
      foaf_givenName: Lisa Annabelle
      foaf_name: Bugnet, Lisa Annabelle
      foaf_surname: Bugnet
      foaf_workInfoHomepage: http://www.librecat.org/personId=d9edb345-f866-11ec-9b37-d119b5234501
    orcid: 0000-0003-0142-4000
  bibo_doi: 10.1016/b978-0-443-21439-4.00036-5
  bibo_volume: 2
  dct_date: 2026^xs_gYear
  dct_isPartOf:
  - http://id.crossref.org/issn/9780443214400
  dct_language: eng
  dct_publisher: Elsevier@
  dct_title: Asteroseismology@
...