{
  "id": "1602.01800",
  "version": "v1",
  "published": "2016-02-03T13:08:56.000Z",
  "updated": "2016-02-03T13:08:56.000Z",
  "title": "Modelling the flaring emission at the Galactic Centre",
  "authors": [
    "E. M. Howard"
  ],
  "comment": "3 pages, 2 figures, Galactic Center Workshop (19 - 23 October 2009 : Shanghai, China), The Galactic Center: a Window to the Nuclear Environment of Disk Galaxies. Proceedings of a workshop held at Shanghai, China Oct. 19-23, 2009. Ed. M. R. Morris, Q. D. Wang, F. Yuan. Astronomical Society of the Pacific, 2011, p.378",
  "categories": [
    "astro-ph.HE"
  ],
  "abstract": "The massive black hole at the Galactic Centre is known to be variable in radio, millimeter, near-IR and X-rays. We investigate the physical processes responsible for the variable observed emissions from the compact radio source Sgr A*. We study the evolution of the variable emission region and present light curves and time-resolved spectra of emissions from the accretion disk, close to the event horizon, near the marginally stable orbit of a Kerr black hole.",
  "revisions": [
    {
      "version": "v1",
      "updated": "2016-02-03T13:08:56.000Z"
    }
  ],
  "analyses": {
    "keywords": [
      "galactic centre",
      "flaring emission",
      "compact radio source sgr",
      "kerr black hole",
      "event horizon"
    ],
    "note": {
      "typesetting": "TeX",
      "pages": 3,
      "language": "en",
      "license": "arXiv",
      "status": "editable",
      "adsabs": "2011ASPC..439..378H"
    }
  }
}