\begin{table}%t1
\caption{\label{tab:simulfit}Fit results for the RGS~spectra extracted from a 1.1$\arcmin$ wide strip centred on the core of M~87. 
The iron abundance is given with respect to the proto-solar values by \citet{lodders2003}
and the other abundances with respect to iron. Emission measures ($Y = \int n_{{\rm e}} n_{{\rm H}} {\rm d}V$) 
are given in~$10^{64}$~cm$^{-3}$.}
\small%\centering
\par
\begin{tabular}{lccc}
\hline\hline
Parameter 	& 2T-model	& {\it wdem}-model	 \\
\hline
$Y_1$ 		& $0.86\pm0.03$		&		 \\
$Y_2$ 		& $9.97\pm0.13$		&		 \\
$Y_{{\rm wdem}}$&      	& $11.56\pm0.17$		 \\
$kT_1$ (keV)    & $0.80\pm0.01$		& 			 \\  
$kT_2$ (keV)	& $1.67\pm0.02$		&			 \\
$kT_{{\rm max}}$ & 		& $2.38\pm0.05$		 \\
$\alpha$	& 		& $0.47\pm0.02$	 	\\
c		& 		& $0.22\pm0.01$ 		\\
$kT_{{\rm mean}}$ &    	& $1.82\pm0.04$	 		\\
C/Fe		&  $0.73\pm0.11$& $0.74\pm0.13$ 		\\ 
N/Fe		&  $1.62\pm0.19$& $1.62\pm0.21$ 		\\  
O/Fe 		&  $0.60\pm0.03$& $0.59\pm0.04$ 		\\
Ne/Fe		&  $1.40\pm0.11$& $1.25\pm0.12$ 		\\
Mg/Fe		&  $0.70\pm0.05$& $0.60\pm0.06$ 		\\
Fe		&  $0.98\pm0.02$& $1.06\pm0.03$ 		\\
\hline\noalign{\smallskip}
$\chi^2$ / $\nu$ &  2737/1905 		&  2728/1905 	\\
\hline
\end{tabular}
\end{table}