\begin{table}%t7
%\centering
\par
\caption{\label{ratios}Abundance ratios \citep[relative to][]{Asplund} applying temperature structure-independent linear combinations of coronal emission lines. Values given in brackets for EQ~Peg~A correspond to the quiescent state.}
\begin{tabular}{cccc}
\hline\hline
Ratio	& \multicolumn{2}{c}{EQ Peg A} & EQ Peg B\\
\hline
%relative to Asplund
O/N 	& 0.83~$\pm$~0.20 & (1.00~$\pm$~0.29) & 0.81~$\pm$~0.72\\
Ne/O  & 2.48~$\pm$~0.31 & (2.02~$\pm$~0.16) & 2.18~$\pm$~0.41\\
Mg/Ne & 0.20~$\pm$~0.02 & (0.19~$\pm$~0.02) & 0.32~$\pm$~0.07\\
Si/Mg & 2.52~$\pm$~0.21 & (2.56~$\pm$~0.25) & 2.05~$\pm$~0.44\\
S/Si	& 1.26~$\pm$~0.20 &-- 		&--\\
Ne/Fe	& 7.30~$\pm$~0.64& (5.99 $\pm$ 0.34)&5.45 $\pm$ 0.78 \\      
Mg/Fe	& 1.27~$\pm$~0.17& (1.09 $\pm$ 0.19)&1.63 $\pm$  0.43\\  
\hline
\end{tabular}
\end{table}