\begin{table}%t7
\caption{Comparison of NGC~2004 analyses in this paper with that from 
\citet[~K00]{korn00}. In K00, NGC~2004-022 is labeled with the \citet{r74}
 identification~-- B30. K00 use LTE model atmospheres with NLTE line formations. Abundances are presented as [X]~= 12~+ $\log$~([X/H]) in units of dex. }\label{ngc2004comp}   
%\centering
\small
\begin{tabular}{lcc} 
\hline \hline
        &\multicolumn{2}{c}{NGC~2004-022}     \\
        & This paper      &  K00            \\
\hline 
\teff\  (K)	      &    21~780	&    23~450	  \\
\logg\  (cm~s$^{-2}$)   &     3.15	&     3.45	  \\
\eps\   (\kms)	      &       11	&	14	  \\
     	&                 &                 \\
C    	&  7.32           & 7.60:           \\
N    	& 7.68 $\pm$ 0.11 & 7.50 $\pm$ 0.20 \\
O    	& 8.55 $\pm$ 0.27 & 8.35 $\pm$ 0.20 \\
Mg   	& 6.94 $\pm$ 0.19 & 7.00 $\pm$ 0.30 \\
Si   	& 7.23 $\pm$ 0.58 & 6.90 $\pm$ 0.20 \\  				     
Fe   	& 7.00 $\pm$ 0.22 & 7.08 $\pm$ 0.30 \\  			\hline			  
\end{tabular}			  
\end{table}