Modelling the flare activity of Sgr A*

Details Modelling the flare activity of Sgr A* Modelling the flare activity of Sgr A*

Oct 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aipc.1178...50h&link_type=abstract

5TH INTERNATIONAL WORKSHOP ON THE DARK SIDE OF THE UNIVERSE. AIP Conference Proceedings, Volume 1178, pp. 50-56 (2009).

Physics

Accretion Disks, Dark Matter, Black Holes, X-Ray Spectra, Infall, Accretion, And Accretion Disks, Dark Matter, Galactic Nuclei, Circumnuclear Matter, And Bulges, X-Ray

Scientific paper

Latest observational data provides evidence that the emissions from Sgr A* originate from an accretion disc within ten gravitational radii of the dynamical centre of Milky Way. 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 analyse light curves and time-resolved spectra of emissions originated at the surface of the accretion disk, close to the event horizon, near the marginally stable orbit of a Kerr black hole.

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