{
  "id": "1706.07020",
  "version": "v1",
  "published": "2017-06-21T17:29:01.000Z",
  "updated": "2017-06-21T17:29:01.000Z",
  "title": "Pulsating White Dwarfs",
  "authors": [
    "S. O. Kepler",
    "Alejandra D. Romero"
  ],
  "comment": "10 pages, 2 figures, Wide-field variability surveys: a 21st-century perspective, 22nd Los Alamos Stellar Pulsation Conference Series meeting, San Pedro de Atacama, Chile, Nov. 28 - Dec. 2, 2016",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The Sloan Digital Sky Survey has allowed us to increase the number of known white dwarfs by a factor of five and consequently the number of known pulsating white dwarfs also by a factor of five. It has also led to the discovery of new types of variable white dwarfs, as the variable hot DQs, and the pulsating Extremely Low Mass white dwarfs. With the Kepler Mission, it has been possible to discover new phenomena, the outbursts present in a few pulsating white dwarfs.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2017-06-21T17:29:01.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "pulsating white dwarfs",
      "sloan digital sky survey",
      "extremely low mass white dwarfs",
      "pulsating extremely low mass white",
      "variable white dwarfs"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}