Active Galactic Nuclei-Plasma around Super-massive Black Hole

Details Active Galactic Nuclei-Plasma around Super-massive Black Hole Active Galactic Nuclei-Plasma around Super-massive Black Hole

Apr 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1121...71p&link_type=abstract

SPACE PLASMA PHYSICS: School of Space Plasma Physics. AIP Conference Proceedings, Volume 1121, pp. 71-77 (2009).

Physics

Plasma Physics

Black Holes, Galaxy Clusters, X-Ray Binaries, Infall, Accretion, And Accretion Disks, Astronomical And Space-Research Instrumentation

Scientific paper

Active Galactic Nuclei (AGN) are the most luminous objects in the Universe. It is widely accepted that radiation emitted from these objects originates in an accretion disk around a Supermassive Black Hole (SMBH). Emission spectral lines (in the X-ray and UV/optical) are used to investigate the plasma conditions in the vicinity of the SMBH. Here we give a short overview of the emission line profiles and their usage for determination of kinematics (geometry) of emitting plasma around black hole.

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