\begin{table}%T1
%\centering
\par
\caption{
  Consequences for the CRp scaling parameter $X_\CRp$ and $\tilde{n}_{\CRp,0}$
  by comparing the integrated flux above 730 GeV to HEGRA data of the radio
  galaxy M~87 within the innermost two data points corresponding to $\theta =
  0.126\degr$. The spatial distribution of CRp is given by the isobaric,
  the adiabatic, and the diffusion model, respectively (see
  Sect.~\ref{CRpdistribution}). 
  In the first two cases the values are calculated for a CRp population with
  and without lower cutoff $p_{\rm min}$ while in the latter case two
  different lifetimes of the source have been considered. Note that the
  averaged CRp luminosity $L_\CRp$ scales with $\kappa_{29} = \kappa/(10^{29}
  \mbox{ cm}^2 \mbox{ s}^{-1})$.} \label{tab:Xcrp}
  $$ 
\begin{tabular}{lcccc}
\hline \hline
\vphantom{\Large A}%
$\alpha_{\rm GeV}^{\rm TeV}$ 
& $X_\CRp^{\rm isobaric}$ & $X_\CRp^{\rm adiabatic}$
& $\tilde{n}_{\CRp,0}~[\mbox{cm}^{-3}]$
& $L_\CRp~\left[\kappa_{29}\mbox{ erg}/\mbox{s}\right]$ \\
\par
\hline 
& \multicolumn{2}{l}{\underline{$p_{\rm min} = 0\mbox{ GeV} c^{-1}:$}}
& \multicolumn{2}{l}{\underline{$t = 1\mbox{ Gyr }\kappa_{29}^{-1}:$}}
\vphantom{\Large A} \\
\vphantom{\Large A}%
2.1  & 0.47 & 0.31 & $1.8 \times 10^{-7}$ & $1.1 \times 10^{43}$ \\
2.2  & 0.65 & 0.43 & $5.0 \times 10^{-7}$ & $1.6 \times 10^{43}$ \\
2.27 & 0.99 & 0.64 & $1.0 \times 10^{-6}$ & $2.4 \times 10^{43}$ \\
\hline 
& \multicolumn{2}{l}{\underline{$p_{\rm min} = 2\mbox{ GeV} c^{-1}:$}}
& \multicolumn{2}{l}{\underline{$t = 3\mbox{ Gyr }\kappa_{29}^{-1}:$}}
\vphantom{\Large A} \\
\vphantom{\Large A}%
2.1  & 0.42 & 0.28 & $1.2 \times 10^{-7}$ & $7.6 \times 10^{42}$ \\
2.2  & 0.52 & 0.34 & $3.4 \times 10^{-7}$ & $1.1 \times 10^{43}$ \\
2.27 & 0.73 & 0.47 & $6.8 \times 10^{-7}$ & $1.6 \times 10^{43}$ \\
\par
\hline 
\end{tabular}
$$
\end{table}