The Appearance of Sgr A* from GRMHD Simulations

Details The Appearance of Sgr A* from GRMHD Simulations The Appearance of Sgr A* from GRMHD Simulations

Jan 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009aas...21341105d&link_type=abstract

American Astronomical Society, AAS Meeting #213, #411.05; Bulletin of the American Astronomical Society, Vol. 41, p.216

Astronomy and Astrophysics

Astronomy

Scientific paper

New time-dependent, 3D GRMHD simulations possess tremendous potential for testing strong field general relativity and advancing our understanding of accreting black hole systems. However, detailed analyses comparing the results of such simulations with observations are lacking. I present results from the application of a new, analytic ray tracing code to tilted disk simulations, and compare the predictions with current and future observations of Sgr A*.

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