{
  "id": "1308.1626",
  "version": "v1",
  "published": "2013-08-07T16:25:15.000Z",
  "updated": "2013-08-07T16:25:15.000Z",
  "title": "Time-dependent modelling of pulsar wind nebulae",
  "authors": [
    "M. J. Vorster",
    "O. Tibolla",
    "S. E. S. Ferreira",
    "S. Kaufmann"
  ],
  "comment": "ICRC 2013 proceedings paper",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "A spatially-independent model that can be used to calculate the temporal evolution of the electron/ positron spectrum in a spherically expanding pulsar wind nebula is presented. The model is applied to the young nebula G21.5-0.9, as well as to the unidentified TeV sources HESS J1427-608 and HESS J1507-622. The parameters derived from the model strengthens the idea that the unidentified sources can be identified as evolved pulsar wind nebulae.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2013-08-07T16:25:15.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "time-dependent modelling",
      "evolved pulsar wind nebulae",
      "spherically expanding pulsar wind nebula",
      "young nebula g21",
      "unidentified tev sources hess"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1246885,
      "adsabs": "2013arXiv1308.1626V"
    }
  }
}