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Modelling the flaring emission at the Galactic Centre by Howard, E. M. is a scholarly article available to read on EtoBox.

What is Modelling the flaring emission at the Galactic Centre about?

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.

Author

Howard, E. M.

Published

2016

Language

EN