{
  "id": "1610.02173",
  "version": "v1",
  "published": "2016-10-07T08:11:07.000Z",
  "updated": "2016-10-07T08:11:07.000Z",
  "title": "The Clusters AgeS Experiment (CASE). Variable stars in the field of the globular cluster NGC 362",
  "authors": [
    "M. Rozyczka",
    "I. B. Thompson",
    "W. Narloch",
    "W. Pych",
    "A. Schwarzenberg - Czerny"
  ],
  "comment": "Accepted by Acta Astronomica",
  "categories": [
    "astro-ph.SR"
  ],
  "abstract": "The field of the globular cluster NGC 362 was monitored between 1997 and 2015 in a search for variable stars. BV light curves were obtained for 151 periodic or likely periodic variables, over a hundred of which are new detections. Twelve newly detected variables are proper motion members of the cluster: two SX Phe and two RR Lyr pulsators, one contact binary, three detached or semi-detached eclipsing binaries, and four spotted variables. The most interesting objects among these are the binary blue straggler V20 with an asymmetric light curve, and the 8.1 d semidetached binary V24 located on the red giant branch of NGC 362, which is a Chandra X-ray source. We also provide substantial new data for 24 previously known variables.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-10-07T08:11:07.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "globular cluster ngc",
      "clusters ages experiment",
      "variable stars",
      "binary blue straggler v20",
      "rr lyr pulsators"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}