{
  "id": "1906.07490",
  "version": "v1",
  "published": "2019-06-18T10:52:53.000Z",
  "updated": "2019-06-18T10:52:53.000Z",
  "title": "Short period variable stars in young open cluster Stock 8",
  "authors": [
    "Sneh Lata",
    "Anil. K. Pandey",
    "Ram Kesh Yadav",
    "Andrea Richichi",
    "Puji Irawati",
    "Neelam Panwar",
    "V. S. Dhillon",
    "T. R. Marsh"
  ],
  "comment": "17 pages, 14 figures, Accepted for the publication in Astronomical Journal",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "We present time series photometry in the field of Stock 8 and identified 130 short period variable stars. Twenty eight main-sequence and 23 pre-main-sequence variables are found to be part of cluster Stock 8. The main-sequence variables are classified as slow pulsator of the B type, $\\beta$ Cep and $\\delta$ Scuti stars. Fourteen main-sequence stars could be new class variables as discussed by Mowlavi et al. (2013) and Lata et al. (2014). The age and mass of pre-main-sequence variables are found to be $\\lesssim$ 5 Myr and in the mass range of 0.5 to 2.8 M$_{\\odot}$, respectively. These pre-main-sequence stars could be T-Tauri variables. We have found 5 and 2 of 23 PMS variables as classical T-Tauri stars and Herbig Ae/Be stars, respectively, whereas 16 PMS stars are classified as weak-line T Tauri stars.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2019-06-18T10:52:53.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "short period variable stars",
      "young open cluster stock",
      "pre-main-sequence variables",
      "time series photometry",
      "herbig ae/be stars"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 17,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}