{
  "id": "1211.7350",
  "version": "v1",
  "published": "2012-11-30T19:40:32.000Z",
  "updated": "2012-11-30T19:40:32.000Z",
  "title": "Extended X-ray emission around RRAT J1819-1458",
  "authors": [
    "A. Camero-Arranz",
    "N. Rea",
    "M. A. McLaughlin",
    "N. Bucciantini",
    "P. Slane",
    "B. Gaensler",
    "D. Torres",
    "L. Stella",
    "E. de Onña",
    "G. Israel",
    "F. Camilo",
    "A. Possenti"
  ],
  "comment": "Proceedings of IAUS 291 \"Neutron Stars and Pulsars: Challenges and Opportunities after 80 years\", J. van Leeuwen (ed.); 4 pages, 3 figures",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "We present new imaging and spectral analysis of the recently discovered extended X-ray emission around the high-magnetic-field rotating radio transient RRAT J1819-1458. We used two Chandra observations, taken on 2008 May 31 and 2011 May 28. The diffuse X-ray emission was detected with a significance of ~19sigma in the image obtained by combining the two observations. Long-term spectral variability has not been observed. Possible scenarios for the origin of this diffuse X-ray emission, further detailed in Camero-Arranz et al. (2012), are here discussed.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2012-11-30T19:40:32.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "extended x-ray emission",
      "diffuse x-ray emission",
      "high-magnetic-field rotating radio transient rrat",
      "long-term spectral variability",
      "spectral analysis"
    ],
    "tags": [
      "journal article"
    ],
    "publication": {
      "doi": "10.1017/S1743921312023800"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 4,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1204971,
      "adsabs": "2013IAUS..291..261C"
    }
  }
}