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M. Georganopoulos (UMBC/ NASA-GSFC), E. S. Perlman (UMBC), D. Kazanas (NASA/GSFC)
In general, a calculation of the synchrotron and inverse Compton emission from a homogeneous source is only amenable to numerical solutions. Here we present simple analytical results for some particular cases that may be useful in the study of non-thermal spectra.
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Bulletin of the American Astronomical Society, 37 #4
© 2005. The American Astronomical Soceity.