{
  "id": "1411.1063",
  "version": "v1",
  "published": "2014-11-04T21:00:12.000Z",
  "updated": "2014-11-04T21:00:12.000Z",
  "title": "Asteroseismology of Cool Stars",
  "authors": [
    "Daniel Huber"
  ],
  "comment": "13 pages, 7 figures; Proceedings of the 18th Cambridge Workshop on Cool Stars, Stellar Systems, and the Sun, Eds G. van Belle & H. Harris",
  "categories": [
    "astro-ph.SR",
    "astro-ph.EP"
  ],
  "abstract": "The measurement of oscillations excited by surface convection is a powerful method to study the structure and evolution of cool stars. CoRoT and Kepler have initiated a revolution in asteroseismology by detecting oscillations in thousands of stars from the main sequence to the red-giant branch, including a large number of exoplanet host stars. In this contribution I will review recent asteroseismic results, focusing in particular on the internal rotation of red giant stars and the impact of asteroseismology on the characterization of exoplanets.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-11-04T21:00:12.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "cool stars",
      "asteroseismology",
      "exoplanet host stars",
      "red giant stars",
      "surface convection"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 13,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2015csss...18..337H"
    }
  }
}