Skip to main content

Influence of microlensing on the active galactic nucleus Fe Kα line

Buy Article:

$63.00 plus tax (Refund Policy)

We have studied the influence of gravitational microlensing on the Fe Kα line originating from a compact accretion disc of active galactic nuclei. We found that microlensing can produce line profile deformation as well as a significant amplification of the line flux. The line deformation and line flux amplification depend not only on the parameters of the microlens but also on the disc parameters.
No References
No Citations
No Supplementary Data
No Data/Media
No Metrics

Keywords: Gravitational microlensing; Quasars; Spectral line; X-rays

Document Type: Research Article

Affiliations: 1: Astronomical Observatory Volgina 7 11160 Belgrad Serbia 2: Instituto de Astrofísica de Canarias E-382005 La Laguna Tenerife Spain

Publication date: 2003-08-01

More about this publication?
  • Access Key
  • Free content
  • Partial Free content
  • New content
  • Open access content
  • Partial Open access content
  • Subscribed content
  • Partial Subscribed content
  • Free trial content
Cookie Policy
X
Cookie Policy
Ingenta Connect website makes use of cookies so as to keep track of data that you have filled in. I am Happy with this Find out more