{
  "id": "1611.04919",
  "version": "v1",
  "published": "2016-11-15T16:25:19.000Z",
  "updated": "2016-11-15T16:25:19.000Z",
  "title": "The potential of space observations for pulsating pre-main sequence stars",
  "authors": [
    "Konstanze Zwintz"
  ],
  "comment": "4 pages, 2 figures, proceedings of the conference \"Seismology of the Sun and the Distant Stars 2016\", Joint TASC2 & KASC9 Workshop - SPACEINN & HELAS8 Conference",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The first asteroseismic studies of pre-main sequence (pre-MS) pulsators have been conducted based on data from the space telescopes MOST and CoRoT with typical time bases of less than 40 days. With these data, a relation between the pulsational properties of pre-MS delta Scuti stars and their relative evolutionary phase on their way from the birthline to the zero-age main sequence was revealed. But it is evident from comparison with the more evolved pulsators in their main sequence or post-main sequence stages observed by the main Kepler mission, that many more questions could be addressed with significantly longer time bases and ultra-high precision. Here, I will discuss the observational status of pre-MS asteroseismology and the potential of future space observations for this research field.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-11-15T16:25:19.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "pulsating pre-main sequence stars",
      "space observations",
      "pre-ms delta scuti stars",
      "significantly longer time bases",
      "main kepler mission"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}