\begin{table}%t2
\caption{Fit results for spatially-resolved RGS~spectra. We model the plasma with two thermal components. 
Abundances are given with respect to the proto-solar values by \citet{lodders2003}. The emission measures are given in~$10^{64}$~cm$^{-3}$.}
\small%\centering
\par
\begin{tabular}{l|cccc}
\hline\hline
Par.		 & --0.5 / 0.5$\arcmin$  & 0.5 / 1.5$\arcmin$  & 1.5 / 2.5$\arcmin$ & 2.5 / 3.5$\arcmin$  \\
\hline
$Y_1$			 &  $0.82\pm 0.04$ &  $0.23\pm0.03$  &  $0.16\pm0.02$  &  $0.18\pm0.02$  \\
$Y_2$			 &  $10.83\pm0.17$ &  $8.38\pm0.08$  &  $6.18\pm0.10$  &  $4.79\pm0.07$  \\
$kT_1$     		 &  $0.79\pm 0.01$ &  $0.81\pm0.03$  &  $0.69\pm0.02$  &  $0.69\pm0.03$  \\
$kT_2$ 			 &  $1.69\pm 0.03$ &  $1.87\pm0.04$  &  $1.88\pm0.05$  &  $1.66\pm0.05$  \\
C                        &  $0.63\pm 0.16$ &  $0.44\pm0.13$  &  $0.30\pm0.16$  &  $<$$0.18$  \\
N                        &  $1.64\pm 0.24$ &  $0.62\pm0.18$  &  $0.67\pm0.22$  &  $<$$0.23$	\\
O			 &  $0.58\pm 0.03$ &  $0.48\pm0.02$  &  $0.52\pm0.03$  &  $0.45\pm0.03$  \\
Ne			 &  $1.41\pm 0.12$ &  $1.17\pm0.13$  &  $0.89\pm0.17$  &  $<$$0.23$	\\
Fe			 &  $0.95\pm 0.03$ &  $0.78\pm0.03$  &  $0.65\pm0.03$  &  $0.50\pm0.03$  \\
Scale $s$		 &  $2.14\pm 0.10$ &  $1.10\pm0.05$  &  $1.18\pm0.09$  &  $1.42\pm0.08$  \\
\hline
$\chi^2$ / $\nu$	 &  1308/918    &  1265/918   &  1199/918  & 1187/918	 \\
\hline
\end{tabular}
\label{tabprof}
\end{table}