\begin{table}%t2
 \caption{\label{t2}Relative intensities of prominent emission lines of V838 Her on
1991 April 2.}
%\centering
\par
 \begin{tabular}{crl}
 \hline \hline\noalign{\smallskip}
$\lambda_{\rm obs}$ & Int. & ident.  \\
 (\AA) &  &  \\
  \hline
3966 & 26.0: & H$\epsilon$, [Ne III] 3967.5 \\
4051 & 1.0 & C III 24, 4056.1 \\
4101 & 36.2 &  H$\delta$ \\
4206 & 0.8 & C IV 11, 4217 \\
4248 & 2.8 & C II 6, 4267.0, 4267.3 \\
4341 & 47.5 &  H$\gamma$ \\
4467  & 5.9 & He I 4471 \\
4611  & 2.9 & N II 5, 4607.2, 4613.9 \\
4647  & 7.5 & N III 2, 4640.6, 4641.9, C III 1, 4650.2\\
4688  & 4.3 & He II 4686 \\
4724  & 1.2: & He I 4713, [Ne IV] 4720 \\
4861  & 100 & H$\beta$ \\
4934  & 1.9: & He 1 4922, Fe II 4924 \\
5027  & 7.2 & C IV 3, 5021,5023, He I 5016, Fe II 5018\\
5076  & 1.1: & Si II 5, 5056? \\
5167  & 2.1 & Fe II 42, 5169.0 \\
5314  & 0.7 & Fe II 49, 5316.6 \\
5468  & 0.8 & N II 2, 5462.6 \\
5675  & 3.5 & N II 3, 5679.6, C III 2, 5696.0 \\
5796  & 1.4: & C IV 1, 5801.5, 5812.1 \\
5872  & 20.2 & He I 5876, C III 20, 5871.6, 5894.1 \\
6129  & 0.7 & C III 13, 6154.4, 6156.6 \\
6268  & 0.2 & blue peak of [S III] 6310 \\
6353  & 6.2 & Si II 2, 6341, 6371 [S III] 6310 \\
6559  & 435 & H$\alpha$ \\
6672  & 5.0: & He I 6678 \\
7060  & 13.2: & He I 7065, C II 20, 7115 \\
\hline
 \end{tabular} 
\tablefoot{The effect of the interstellar extinction is corrected by $E(B-V)=0.53$.}
\end{table}