Changeset 6796 for trunk/MagicSoft

Timestamp:

03/09/05 09:49:48 (20 years ago)

Author:

hbartko

Message:

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File:

• trunk/MagicSoft/GC-Proposal/GC.tex (modified) (1 diff)

trunk/MagicSoft/GC-Proposal/GC.tex

@@ -244 +244 @@
 \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.