{
  "id": "0908.1010",
  "version": "v1",
  "published": "2009-08-07T09:35:04.000Z",
  "updated": "2009-08-07T09:35:04.000Z",
  "title": "Multi-wavelength observations of isolated neutron stars",
  "authors": [
    "Roberto P. Mignani"
  ],
  "comment": "10 pages, 5 figures, To be published in the proceedings of the conference \"Neutron Stars and Gamma Ray Bursts: Recent Developments and Future Directions\" - March 30 - April 4, 2009 (Cairo and Alexandria, Egypt)",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "Forty years elapsed since the optical identification of the first isolated neutron star (INS), the Crab pulsar. 25 INSs have been now identified in the optical (O), near-ultraviolet (nUV), or near-infrared (nIR), hereafter UVOIR, including rotation-powered pulsars (RPPs), magnetars, and X-ray-dim INSs (XDINSs), while deep investigations have been carried out for compact central objects (CCOs), Rotating RAdio transients (RRATs), and high-magnetic field radio pulsars (HBRPs). In this review I describe the status of UVOIR observations of INSs, their emission properties, and I present recent results.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2009-08-07T09:35:04.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "multi-wavelength observations",
      "high-magnetic field radio pulsars",
      "compact central objects",
      "first isolated neutron star",
      "crab pulsar"
    ],
    "tags": [
      "conference paper"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 10,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 828080,
      "adsabs": "2009arXiv0908.1010M"
    }
  }
}