{
  "id": "astro-ph/0005379",
  "version": "v1",
  "published": "2000-05-18T21:12:37.000Z",
  "updated": "2000-05-18T21:12:37.000Z",
  "title": "The Rapidly Fading Afterglow from the Gamma-Ray Burst of 1999 May 6",
  "authors": [
    "G. B. Taylor",
    "J. S. Bloom",
    "D. A. Frail",
    "S. R. Kulkarni",
    "S. G. Djorgovski",
    "B. A. Jacoby"
  ],
  "comment": "in press at ApJ Letters, 13 page LaTeX document includes 2 postscript figures",
  "doi": "10.1086/312760",
  "categories": [
    "astro-ph"
  ],
  "abstract": "We report on the discovery of the radio afterglow from the gamma-ray burst (GRB) of 1999 May 6 (GRB 990506) using the Very Large Array (VLA). The radio afterglow was detected at early times (1.5 days), but began to fade rapidly sometime between 1 and 5 days after the burst. If we attribute the radio emission to the forward shock from an expanding fireball, then this rapid onset of the decay in the radio predicts that the corresponding optical transient began to decay between 1 and 5 minutes after the burst. This could explain why no optical transient for GRB 990506 was detected in spite of numerous searches. The cause of the unusually rapid onset of the decay for the afterglow is probably the result of an isotropically energetic fireball expanding into a low density circumburst environment. At the location of the radio afterglow we find a faint (R ~ 24 mag) host galaxy with a double morphology.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2000-05-18T21:12:37.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "gamma-ray burst",
      "rapidly fading afterglow",
      "radio afterglow",
      "low density circumburst environment",
      "rapid onset"
    ],
    "tags": [
      "journal article"
    ],
    "note": {
      "typesetting": "LaTeX",
      "pages": 13,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "inspire": 545930
    }
  }
}