Radiation spectra from MHD simulations of low angular momentum flows

Details Radiation spectra from MHD simulations of low angular momentum flows Radiation spectra from MHD simulations of low angular momentum flows

Apr 2007

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2007iaus..238..411m&link_type=abstract

Black Holes from Stars to Galaxies -- Across the Range of Masses. Edited by V. Karas and G. Matt. Proceedings of IAU Symposium #

Physics

Scientific paper

We performed Monte Carlo simulations for calculations of radiation spectra from magnetohydrodynamic simulations of low angular momentum flows (with angular momentum parameter lambda ˜ 2 Rg c). Calculations of dynamics were performed by Proga et al. (2003). We treat the flow as two temperature flow where electron temperature is calculated from energy balance equation that includes magnetic heating, ion-electrons coupling, cooling in form of synchrotron, bremsstrahlung radiation and advection of heat. As a result we show radiation spectra calculated for two accretion states of magnetized torus which forms in a low angular momentum flows . We also show the radiation intensity maps for such kind of flow for given energy band from radio to X-rays.

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