{
  "id": "2201.11629",
  "version": "v1",
  "published": "2022-01-27T16:35:54.000Z",
  "updated": "2022-01-27T16:35:54.000Z",
  "title": "Asteroseismology across the HR diagram",
  "authors": [
    "Donald Kurtz"
  ],
  "comment": "Manuscript submitted to Annual Reviews of Astronomy and Astrophysics for future publication in Volume 60. This is the author's own version. The final version will become available from https://www.annualreviews.org/journal/astro. 63 pages",
  "categories": [
    "astro-ph.SR",
    "astro-ph.EP"
  ],
  "abstract": "Asteroseismology has grown from its beginnings three decades ago to a mature field teeming with discoveries and applications. This phenomenal growth has been enabled by space photometry with precision $10-100$ times better than ground-based observations, with nearly continuous light curves for durations of weeks to years, and by large scale ground-based surveys spanning years designed to detect all time-variable phenomena. The new high precision data are full of surprises, deepening our understanding of the physics of stars. $\\bullet$ This review explores asteroseismic developments from the last decade primarily as a result of light curves from the Kepler and TESS space missions for: massive upper main-sequence OBAF stars, pre-main-sequence stars, peculiar stars, classical pulsators, white dwarfs and subdwarfs, and tidally interacting close binaries. $\\bullet$ The space missions have increased the numbers of pulsators in many classes by an order of magnitude. $\\bullet$ Asteroseismology measures fundamental stellar parameters and stellar interior physics - mass, radius, age, metallicity, luminosity, distance, magnetic fields, interior rotation, angular momentum transfer, convective overshoot, core burning stage - supporting disparate fields such as galactic archeology, exoplanet host stars, supernovae progenitors, gamma ray and gravitational wave precursors, close binary star origins and evolution, and standard candles. $\\bullet$ Stars are the luminous tracers of the universe. Asteroseismology significantly improves models of stellar structure and evolution on which all inference from stars depends.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2022-01-27T16:35:54.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "hr diagram",
      "scale ground-based surveys spanning",
      "asteroseismology measures fundamental stellar parameters",
      "massive upper main-sequence obaf stars",
      "light curves"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 63,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}