{
  "id": "1810.02257",
  "version": "v1",
  "published": "2018-10-04T14:56:15.000Z",
  "updated": "2018-10-04T14:56:15.000Z",
  "title": "Neutron stars as sources of gravitational waves",
  "authors": [
    "Michał Bejger"
  ],
  "comment": "6 pages; contribution to XXXVIII Polish Astronomical Society meeting, Zielona G\\'ora, 11-14 September 2017",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The global network of ground-based gravitational-wave detectors (the Advanced LIGO and the Advanced Virgo) is sensitive at the frequency range corresponding to relativistic stellar-mass compact objects. Among the promising types of gravitational-wave sources are binary systems and rotating, deformed neutron stars. I will describe these sources and present predictions of how their observations will contribute to modern astrophysics in the near future.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2018-10-04T14:56:15.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gravitational waves",
      "relativistic stellar-mass compact objects",
      "deformed neutron stars",
      "global network",
      "ground-based gravitational-wave detectors"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 6,
      "language": "en",
      "license": "arXiv",
      "status": "editable"
    }
  }
}