{
  "id": "astro-ph/9911032",
  "version": "v1",
  "published": "1999-11-03T10:53:53.000Z",
  "updated": "1999-11-03T10:53:53.000Z",
  "title": "A comparison of radio emission from neutron star and black hole X-ray binaries",
  "authors": [
    "R. P. Fender"
  ],
  "comment": "To be published in Proc. NATO advanced study institute `The Neutron Star - Black Hole connection'",
  "categories": [
    "astro-ph"
  ],
  "abstract": "I compare the properties of radio emission from neutron star and black hole X-ray binaries. In both transient and persistent systems the ratio of X-ray : radio fluxes is comparable for (low field) neutron stars and black holes. It appears that, broadly speaking, the disc : jet coupling is independent of the nature of the accretor, (except for X-ray pulsars where the strong magnetic field prevents formation of an inner accretion disc and jet).",
  "revisions": [
    {
      "version": "v1",
      "updated": "1999-11-03T10:53:53.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "black hole x-ray binaries",
      "neutron star",
      "radio emission",
      "strong magnetic field prevents formation",
      "comparison"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 0,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 520115,
      "adsabs": "1999astro.ph.11032F"
    }
  }
}