\begin{table}%T2
\caption{Results of the {\it IUE} measurements for RS~CVn stars.}\label{tab:data2}
%\centerline
{
\begin{tabular}{@{} r l r r r r r r r r r}
\hline \hline \noalign{\smallskip}
HIP  & Name  & & $M_{\rm V}(IUE)$ & $\Delta M_{\rm V}(IUE)$ & ${\rm log}~W_{\circ}$ & $\Delta {\rm log}~W_{\circ}$ & & ${\rm log}~L_{\mbox{\ion{Mg}{ii}}}$ & $\Delta {\rm log}~L_{\mbox{\ion{Mg}{ii}}}$ &
$N$  \\\noalign{\smallskip}
\hline \noalign{\smallskip}
  4157 & CF Tuc       &  &   2.76 &   0.17 &   2.16 &   0.15 &  &  30.41 &   0.30 &    8  \\
  9630 & XX Tri       &  &   1.86 &        &   2.07 &        &  &  31.23 &         &    1  \\
 10280 & TZ Tri       &  &   0.16 &   0.05 &   2.19 &   0.02 &  &  31.21 &   0.08 &    3  \\
 13118 & VY Ari       &  &   3.59 &   0.17 &   1.91 &   0.01 &  &  30.13 &   0.06 &    5  \\
%% 13402 & EP Eri       &  &   5.92 &   0.13 &   1.71 &   0.08 &  &  28.77 &   0.20 &    7 & \\
 16042 & UX Ari       &  &   2.89 &   0.43 &   2.09 &   0.30 &  &  30.60 &   0.53 &   65  \\
 16846 & V711 Tau     &  &   3.45 &   0.46 &   2.10 &   0.48 &  &  30.45 &   0.46 &  264  \\
 19431 & EI Eri       &  &   3.29 &   0.16 &   2.12 &   0.23 &  &  30.23 &   0.18 &   28  \\
 23743 & BM Cam       &  &  --0.32 &   0.10 &   2.23 &   0.01 &  &  31.77 &   0.08 &    2  \\
 24608 & $\alpha$ Aur &  &  --0.45 &   0.22 &   2.16 &   0.23 &  &  31.06 &   0.15 &   76  \\
 35600 & AR Mon       &  &   1.43 &        &   2.41 &        &  &  30.99 &         &    1  \\
 37629 & $\sigma$ Gem &  &   1.36 &   0.26 &   2.13 &   0.30 &  &  31.09 &   0.33 &   27  \\
 46159 & IL Hya       &  &   2.15 &        &   2.02 &        &  &  30.89 &         &    1  \\
 56851 & V829 Cen     &  &        &        &   1.99 &        &  &  30.67 &         &    1  \\
 59600 & HU Vir       &  &   3.25 &        &   2.04 &        &  &  30.46 &         &    1  \\
 59796 & DK Dra       &  &   0.50 &   0.14 &   2.12 &   0.13 &  &  31.40 &   0.14 &    4  \\
 64293 & RS~CVn       &  &   2.98 &   0.14 &   2.05 &   0.05 &  &  29.96 &   0.08 &    3  \\
 65187 & BM CVn       &  &        &        &   2.06 &        &  &  30.89 &         &    1  \\
 81519 & WW Dra       &  &   3.10 &        &   2.28 &        &  &  29.97 &         &    1  \\
 82080 & $\varepsilon$ UMi  &  &  --0.94 &   0.00 &   2.15 &   0.10 &  &  31.39 &   0.08 &    2  \\
 84586 & V824 Ara     &  &   4.30 &   0.07 &   2.13 &   0.05 &  &  30.05 &   0.33 &    3  \\
 85852 & DR Dra       &  &   1.62 &        &   2.05 &        &  &  30.88 &         &    1  \\
 87965 & Z Her        &  &   2.29 &        &   1.82 &        &  &  29.92 &         &    1  \\
 88848 & V815 Her     &  &   5.10 &   0.05 &   1.87 &   0.16 &  &  29.33 &   0.10 &    4  \\
 94013 & V1762 Cyg    &  &   1.76 &   0.19 &   2.09 &   0.04 &  &  30.98 &   0.06 &    4  \\
 95244 & V4138 Sgr    &  &   2.17 &        &   1.92 &        &  &  30.76 &         &    1  \\
 96003 & V1817 Cyg    &  &  --1.23 &        &   2.22 &        &  &  32.11 &         &    1  \\
 96467 & V1764 Cyg    &  &   0.35 &        &   2.34 &        &  &  31.53 &         &    1  \\
109002 & HK Lac       &  &   1.03 &   0.13 &   2.14 &   0.07 &  &  31.36 &   0.20 &    4  \\
109303 & AR~Lac       &  &   3.08 &   0.90 &   2.28 &   0.33 &  &  30.19 &   0.47 &  198  \\
111072 & V350 Lac     &  &   1.03 &   0.05 &   2.16 &   0.09 &  &  30.97 &   0.11 &    2  \\
112997 & IM Peg       &  &   0.94 &   0.22 &   2.15 &   0.17 &  &  31.34 &   0.20 &   12  \\
114639 & SZ Psc       &  &   2.64 &   0.33 &   2.22 &   0.17 &  &  30.54 &   0.23 &   25  \\
%%115147 & V368 Cep     &  &   6.09 &   0.13 &   1.67 &   0.07 &  &  28.96 &   0.06 &    7 & \\
116584 & $\lambda$ And      &  &   1.75 &   0.35 &   2.01 &   0.22 &  &  30.90 &   0.33 &   79  \\
117915 & II Peg       &  &   4.33 &   0.44 &   1.94 &   0.33 &  &  30.07 &   0.45 &   59  \\
\hline 
%\end{flushleft}
\end{tabular}}
\par
\medskip
{\it Notes}: 
$M_{\rm V}(IUE)$ and $\Delta M_{\rm V}(IUE)$
are the mean visual absolute magnitude and its maximum amplitude. ${\rm log}~
W_{\circ}$ and $\Delta {\rm log}~ W_{\circ}$ are, respectively, the logarithm of the mean
full-width at half-maximum for the \ion{Mg}{ii} line and the
corresponding spread.  ${\rm log}~L_{\mbox{\ion{Mg}{ii}}}$ and $\Delta
{\rm log}~L_{\mbox{\ion{Mg}{ii}}}$ are, respectively, the logarithm of the mean
luminosity of the \ion{Mg}{ii} line and its spread. $N$ is the number
of the spectra used for each star. Units for the line widths~$W_{\circ}$ and
\ion{Mg}{ii} luminosities are in km~s$^{-1}$ and erg~s$^{-1}$,
respectively.
\end{table}