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astro-ph2005
How is the blazar GeV emission really produced?
Markos Georganopoulos, Eric Perlman, Demosthenes Kazanas +1
We show that the external Compton (EC) model for the production of the GeV emission in blazars makes specific predictions for the spectrum and variability of those blazars characte…
astro-ph1997
Modeling the Hard X-Ray Lag and Energy Spectrum of Cyg X-1
Xin-Min Hua, Demosthenes Kazanas, Wei Cui
In an effort to model the observed energy spectrum of Cygnus X-1 as well as its hard X-ray lag by Comptonization in inhomogeneous clouds of hot electrons with spherical geometry an…