Monte Carlo Simulations of High Energy Radiation from Compact Objects

Details Monte Carlo Simulations of High Energy Radiation from Compact Objects Monte Carlo Simulations of High Energy Radiation from Compact Objects

Dec 1999

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1999aas...195.9101l&link_type=abstract

American Astronomical Society, 195th AAS Meeting, #91.01; Bulletin of the American Astronomical Society, Vol. 31, p.1510

Astronomy and Astrophysics

Astronomy

Scientific paper

We report results of Monte Carlo simulations of x-and-gamma-ray emissions from accreting black holes candidates. As seed photons for Comptonization, we use both internal synchrotron photons and external blackbody photons, either from embedded cool blobs, or a central Shakura-Sunyaev optically thick disk. We include radiation from both thermal and nonthermal leptons. The nonthermal leptons are accelerated stochastically by wave turbulence and cooled by coubomb and radiative processes. Both spectra and energy-dependent time variabilities (power density spectra, hard-lags, coherence etc) will be presented.

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