{
  "id": "1501.00498",
  "version": "v1",
  "published": "2014-12-30T08:17:26.000Z",
  "updated": "2014-12-30T08:17:26.000Z",
  "title": "Using radio jets of PKS J0334-3900 to probe the intra-cluster medium in A3135",
  "authors": [
    "L. Pratley",
    "M. Johnston-Hollitt",
    "S. Dehghan",
    "M. Sun"
  ],
  "comment": "To appear in the Proceedings of the IAU Symposium No. 313: Extragalactic jets from every angle, Galapagos, Ecuador, 15-19 September 2014, F. Massaro, C. C. Cheung, E. Lopez, and A. Siemiginowska (Eds.), Cambridge University Press",
  "categories": [
    "astro-ph.GA",
    "astro-ph.HE"
  ],
  "abstract": "We present a multi-wavelength study of the radio galaxy PKS J0334-3900, which resides at the centre of Abell 3135. Using Australia Telescope Compact Array (ATCA) observations at 1.4, 2.5, 4.6 & 8.6 GHz, we performed a detailed analysis of PKS J0334-3900. The morphology and spectral indices give physical parameters that constrain the dynamical history of the galaxy, which we use to produce a simulation of PKS J0334-3900. This simulation shows that the morphology can be generated by a wind in the intracluster medium (ICM), orbital motion caused by a companion galaxy, and precession of the black hole (BH).",
  "revisions": [
    {
      "version": "v1",
      "updated": "2014-12-30T08:17:26.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "radio jets",
      "intra-cluster medium",
      "australia telescope compact array",
      "radio galaxy pks",
      "black hole"
    ],
    "publication": {
      "doi": "10.1017/S1743921315002379"
    },
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 1336288
    }
  }
}