Location of Repository

Iron line profiles from black hole accretion discs with spiral velocity structure

By Sean A. Hartnoll and Eric G. Blackman


Active galactic nuclei (AGN) and some X-ray binaries are thought to be powered by accretion onto a central black hole (e.g. Rees 1984). A fluorescent iron Kα emission line with rest energy 6.4 keV is observed in the X-ray spectrum o

Year: 2002
OAI identifier: oai:CiteSeerX.psu:
Provided by: CiteSeerX
Download PDF:
Sorry, we are unable to provide the full text but you may find it at the following location(s):
  • http://citeseerx.ist.psu.edu/v... (external link)
  • http://arxiv.org/pdf/astro-ph/... (external link)
  • Suggested articles

    To submit an update or takedown request for this paper, please submit an Update/Correction/Removal Request.