Investigating M87 through GRMHD and Novel Monte Carlo Radiation Transport Tools

Details Investigating M87 through GRMHD and Novel Monte Carlo Radiation Transport Tools Investigating M87 through GRMHD and Novel Monte Carlo Radiation Transport Tools

Sep 2011

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2011head...12.3513h&link_type=abstract

American Astronomical Society, HEAD meeting #12, #35.13

Astronomy and Astrophysics

Astronomy

Scientific paper

Results from general relativistic magneto-hydrodynamic simulations of M87 are presented. Spectra are obtained through the use of a unique Monte Carlo radiation transport code, specialized to consider radiation in a region of high velocity shear and magnetic field anisotropy. Ramifications for constraints on physical parameters, such as black hole spin and flare mechanism, will be discussed.

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