{
  "id": "1110.5012",
  "version": "v1",
  "published": "2011-10-23T01:26:40.000Z",
  "updated": "2011-10-23T01:26:40.000Z",
  "title": "Kepler asteroseismology of red-giant stars",
  "authors": [
    "J. Christensen-Dalsgaard"
  ],
  "comment": "To appear in Proceedings of the 61st Fujihara Seminar: Progress in solar/stellar physics with helio- and asteroseismology. H. Shibahashi, ed., ASP Conf. Ser",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The Kepler mission, launched in March 2009, has revolutionized asteroseismology, providing detailed observations of thousands of stars. This has allowed in-depth analysis of stars ranging from compact hot subdwarfs to red giants, and including the detection of solar-like oscillations in hundreds of stars on or near the main sequence. Here I mainly consider solar-like oscillations in red giants, where Kepler observations are yielding results of a perhaps unexpected richness. In addition to giving a brief overview of the observational and numerical results for these stars, I present a simple analysis which captures some of the properties of the observed frequencies.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2011-10-23T01:26:40.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "red-giant stars",
      "kepler asteroseismology",
      "solar-like oscillations",
      "compact hot subdwarfs",
      "red giants"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 941541,
      "adsabs": "2012ASPC..462..503C"
    }
  }
}