{
  "id": "astro-ph/9712254",
  "version": "v1",
  "published": "1997-12-18T17:22:00.000Z",
  "updated": "1997-12-18T17:22:00.000Z",
  "title": "Recent Results on the Anomalous X-ray Pulsars",
  "authors": [
    "S. Mereghetti",
    "L. Stella",
    "G. L. Israel"
  ],
  "comment": "4 pages, 1 figures. To appear in The Active X-ray Sky: Results from BeppoSAX and Rossi-XTE, Nuclear Physics B Proceedings Supplements, L. Scarsi, H. Bradt, P. Giommi and F. Fiore (eds.), Elsevier Science B.V",
  "categories": [
    "astro-ph"
  ],
  "abstract": "The ''Anomalous X-ray Pulsars'' (AXPs) are a small group of X-ray pulsars characterized by periods in the 5-10 s range and by the absence of massive companion stars. There are now 7 possible members of this class of objects. We review recent observational results on their X-ray spectra, spin period evolution, and searches for orbital motion and discuss the implications for possible models.",
  "revisions": [
    {
      "version": "v1",
      "updated": "1997-12-18T17:22:00.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "anomalous x-ray pulsars",
      "spin period evolution",
      "orbital motion",
      "small group",
      "observational results"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1016/S0920-5632(98)00220-5"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 453538
    }
  }
}