Index: /trunk/MagicSoft/GC-Proposal/GC.tex
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--- /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6795)
+++ /trunk/MagicSoft/GC-Proposal/GC.tex	(revision 6796)
@@ -244,5 +244,5 @@
 \subsubsection{Leptonic Models}
 
-Advection dominated accretion flow models, \cite{Atoyan2004}.
+Also advection dominated accretion flow (ADAF) models can describe the production of high energy gamma radiation in the Galactic Center \cite{Atoyan2004}.
 
 A viable site of acceleration of highly energetic electrons could be the compact region within a few gravitational radii of the black hole. In this case the electrons produce not only curvature radiation, which peaks around 1 GeV, but also inverse Compton gamma rays (produced in the Klein-Nishina regime) with the peak emission around 100 TeV. As these high energy gammas cannot escape the source the observed gamma rays would be due to an electromagnetic cascade.