Table 3: Upper limits on the CRp scaling parameter $X_{\rm CRp}$ by comparing the integrated flux above 100 MeV to EGRET upper limits assuming a $\gamma $-ray spectral index in Dermer's model $\alpha _\gamma =\alpha _{\rm p}$. The spatial distribution of CRp is given by the isobaric and the adiabatic model of CRp, respectively (see Sects. 3.2.1 and 3.2.2).
\begin{displaymath}\begin{tabular}{lc*{8}{c}} \hline \hline \vphantom{\Large A}%... ...1.85 & 1.03 & 1.09 & 1.63 & & & & \\ \par\hline \end{tabular}\end{displaymath}

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