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Paper: |
Modelling the Flaring Emission at the Galactic Centre |
Volume: |
439, The Galactic Center: a Window to the Nuclear Environment of Disk Galaxies |
Page: |
378 |
Authors: |
Howard, E. |
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. |
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