\documentstyle{l-aa}
\begin{document}

\begin{table*}
\caption[]{$\lambda$\,Bootis  stars included in Paper I with 
ultraviolet observations. The {\bf L} and {\bf S}
following the image number indicates the aperture used (Large or Small)}
\label{tab_lb}
\begin{flushleft}
\begin{center}
\footnotesize
\begin{tabular}{llllllll}
\hline\noalign{\smallskip}
Identification & T$_{eff}$& log g & IUE images & \multicolumn{4}{c}{Equivalent width (\AA)} \\
               &This work/Sources&This work& SWP       & 1657\AA $ $ & 1670\AA $ $ 
               & 1741\AA $ $ & 1931\AA\\
              & & &LWP &2800\AA $ $& & & \\
\hline\noalign{\smallskip}
HD 4158 & 6550/--- &3.20&         SWP21388L& ---& ---&  0.95&   3.73\\
HD 6870 & 7300/--- &3.90&         LWP02118L& 8.16&   &       &         \\
        &          &    &     SWP21334L&  6.86&  1.06&  2.07&   4.54     \\
        &          &    &     SWP21334S&  5.80&  2.57&  2.65&   3.90     \\
HD 11413& 7900/8100(1);7950(2)&3.80&SWP43607L&  5.07&  1.11&  2.06&  ---     \\
HD 30422& 7950/8100(1)&4.10&      SWP46036L&  3.79&  1.49& ---&  --- \\
HD 31295& 8775/9100(1);8750(3)&4.15&SWP17883L&  3.20& ---& ---&  ---     \\
        &          &     &    SWP17883S&  4.06&  0.75& ---&  ---     \\
        &          &      &   SWP17884L&  3.00&  0.41&  1.00&   1.17     \\
        &          &       &  SWP17884S&  3.48& ---&  1.16&   2.63     \\
HD 39421& 8250/--- &3.70&         SWP38240L&  3.79&  1.11& ---&  ---     \\
        &          &        & SWP38240S&  3.53&  1.53& ---&   2.43     \\
HD 101108& 7950/---&3.80&    LWP02171L&   9.77&       &    &          \\
        &          &        & LWP02171S&7.93   &       &    &          \\
        &          &        & SWP21396L&  3.83&  1.85&  0.95&   2.27     \\
        &          &        & SWP21396S&  3.59& ---&  1.47&   2.02     \\
HD 105058& 7800/---&3.65&         SWP19129L&  5.00& ---&  1.35&   2.87     \\
HD 106223& 6500/6660(5)&3.50&      SWP08720L& ---& ---&  2.23&   5.08     \\
        &          &        & SWP08720S& ---& ---& ---&   5.19     \\
        &          &        & SWP22388L& ---&  0.90& ---&   3.91     \\
        &          &        & SWP22388S& ---& ---&  1.40&   3.61     \\
HD 107233& 7200/7200(1)&4.00&     SWP48198L&  6.03& ---& ---&   3.57     \\
HD 110411& 8850/9100(1);8970(2)&4.20& SWP19125L&  2.90& ---& ---&   1.77     \\
        &          &        & SWP19125S&  2.38&  0.66&  1.18&   1.75     \\
HD 111786& 7500/7600(1);7450(2)&4.00&SWP19124L&  5.90&  1.43&  1.19&   1.69     \\
        &          &        & SWP19124S&  3.78& ---&  1.08&  ---     \\
HD 125162& 8500/8900(1);8650(3)&4.10&SWP17871L&  2.90& ---& ---&  ---     \\
        &          &        & SWP17871S&  3.49& ---& ---&   1.22     \\
        &          &        & SWP17872L&  2.68& ---&  0.80&   1.87     \\
        &          &        & SWP17872S&  2.67& ---&  1.31&   1.17     \\
HD 141851& 8150/8230(4)&3.85&      SWP38237L&  2.61&  1.69& ---&  ---     \\
        &          &        & SWP38237S& ---& ---& ---&   5.07     \\
        &          &        & SWP38238L&  4.46& ---&  1.31&   1.45     \\
HD 142703& 7200/7400(1);7240(4)&3.95& SWP48196L&  7.66& ---&  2.03&   2.86     \\
HD 149303& 8150/---&3.80&   SWP48075L&  2.22&  1.59&  1.23&   2.04     \\
HD 183324& 8700/9300(1);9260(2)&4.10&SWP46039L&  3.68& ---& ---&  ---     \\
HD 192640& 7900/8100(1);7990(2)&3.90&LWP23062L&   3.63&    &    &          \\
         &         &        & SWP17887L&  4.44& ---&  1.22&   2.58     \\
         &         &        & SWP44622L&  4.37&  0.56&  1.24&   2.03     \\
HD 204041& 8100/8100(1)&3.95&      SWP46040L&  2.72& ---& ---&  ---    \\
HD 221756& 8350/9100(1);9020(2)& 3.85&SWP46038L&  3.04& ---& ---&  ---     \\
\hline\noalign{\smallskip}
\end{tabular}
\end{center}

\vspace{0.1cm}

\footnotesize {\bf Sources for T$_{eff}$}: {\bf 1:} Iliev \& Barzova (1995); 
{\bf 2:} St\"urenburg (1993); {\bf 3:} Venn \& Lambert (1990); {\bf 4:} 
North et al. (1994); \mbox{{\bf 5:} Cacciari et al. (1987)}
\end{flushleft}
\end{table*}

\begin{table*}[htb]
\caption[]{Same as Tab. 1 but for the field horizontal branch stars}
\label{tab_fhb}
\begin{flushleft}
\footnotesize
\begin{center}
\begin{tabular}{llllllll}
\hline\noalign{\smallskip}
Identification & $T_{eff}$&log g & IUE images & \multicolumn{4}{c}{Equivalent
width (\AA)} \\
               & & & SWP       & 1657\AA $ $ & 1670\AA $ $
               & 1741\AA $ $ & 1931\AA\\
              &  & & LWP       &2800\AA $ $ & & & \\
\hline\noalign{\smallskip}
Feige 41 & 9800(1) &4.25 (1) & SWP09523L& 1.45&  1.72&  1.49&  1.30\\
HD 60778 & 7722(4) & 2.90 (2)& SWP07351L & 1.82&  2.01&  0.83&  1.53\\
         &         & & SWP07351S & 2.14& ---&  1.23& ---\\
HD 109995& 8300(1),8300(2),8255(4) & 3.36 (2)& LWP03637L &4.34& & & \\ 
         &         &                 & SWP23295L & 1.11& ---&  1.55& ---\\
         &         &                 & SWP23296L & 1.30&  0.56&  0.90&  0.68\\
         &         &                & SWP03932L & 1.43& ---& ---& ---\\
         &         &                & SWP03932S & 1.77& ---&  1.16&  1.49\\
         &         &                & SWP03289L &---&  0.75& ---& ---\\
HD 117880& 8800(1) & 3.80 (2)                & SWP23442L & 1.42& ---&  0.87&
 ---\\
HD 130095&9300(1),8800(2),8300(3)& 3.64 (2)  & SWP03920L & 0.94&  1.09& ---& ---\\
HD 161817&7700(1),7500(2),7580(4)& 3.00 (2)  & SWP03923L & 1.50&  1.29&  1.67& ---\\
\hline\noalign{\smallskip}
\end{tabular}
\end{center}

\vspace{0.1cm}

\footnotesize {\bf Sources for T$_{eff}$}:{\bf 1:} Huenemoerder et al. (1984);
{\bf 2:} De Boer et al. (1997); {\bf 3:} Adelman \& Philip (1990); 
{\bf 4:} Hayes \& Philip (1988).\\
{\bf Sources for log g}:{\bf 1:} Huenemoerder et al. (1984); {\bf 2:} Hayes \& Philip (1988).
\end{flushleft}
\end{table*}


\begin{table*}
\caption[]{Same as Tab. 1 but for the standard stars}
\label{tab_std}
\begin{flushleft}
\footnotesize
\begin{center}
\begin{tabular}{llllllll}
\hline
Identification &T$_{eff}$&log g & IUE images & \multicolumn{4}{c}{Equivalent 
width (\AA)} \\
             &This work/Sources &This work& SWP       & 1657\AA $ $ & 1670\AA $ $ 
& 1741\AA $ $ & 1931\AA\\
              & && LWP       &2800\AA $ $ & & & \\
\hline
HD 1280& 8950/8970(8)  & 3.95 & SWP43462L&  2.21 & 3.05  & 0.87 & 1.62 \\
HD 11636&8400/9000(11) & 4.10 & LWP14036L& 10.55 & & & \\
        &              &      & LWP16921L& 9.18  & & & \\
        &              &      & SWP34228L&  2.99 & 3.01  & 2.00 & 2.09 \\
        &              &      & SWP34229L&  3.75 & 3.16  & 1.86 & 2.51 \\
        &              &      & SWP34872L& ---&  3.91 & 1.91 & 2.69 \\
HD 27176&7400/7350(14) & 4.00 & SWP15538L&  5.18 & 3.14  & 2.60 & 3.06 \\
HD 28052&7350/7370(7)  & 3.50 & SWP09855S& ---&  3.32 &1.88&  5.25 \\
HD 28319&7900/7830(6);7960(7)& 3.75& SWP18390L&  3.74 & 4.71  &1.99& ---\\
        &                    &     & SWP18390S&  3.62 & 2.99  & 2.24 & 4.51\\
HD 28527&8150/8190(7)& 3.90  &  SWP19459L&  5.05 & 4.65  & 2.07 & 4.11\\
HD 28556&7700/7660(7)& 4.10  &  SWP32101L&  3.15 & 3.16  & ---&  4.28\\
HD 41695&8400/---    & 3.90  & SWP03530S& ---&  3.21 & ---& ---\\
HD 48915&9900/9940(14)&4.20  & SWP31909L&  3.00 & 1.74 & ---& ---\\
        &             &      & SWP31910L&  1.39 & 2.14 & 0.94&  0.83\\
        &             &      & SWP31911L&  0.96 & 1.89& --- & 0.80\\
HD 50241&7550/---     &3.50  & SWP28720L&  1.08 & 1.96&  2.78& ---\\
HD 76644&8100/7840(8);7860(6)&4.25& SWP10284L&  5.58 & 3.33&1.95&  3.52\\
        &             &      &SWP13938L&  2.76 & 1.82& ---&  4.55\\
        &             &      &SWP13938S&  4.02 & 2.80& ---&  4.56\\
HD 90132& 7500/---    &3.90  & SWP45006L&  2.93 & 2.86& ---&  1.63\\
        &             &      & SWP28722L&  3.34 & 2.83&2.59&  4.26\\
HD 97603& 8450/8300(8);8400(5)&3.90& SWP19247L&  4.68 &---&  1.69&  3.27\\
        &                     &    & SWP19247S&  3.68 & 3.53& ---&  2.55\\
HD 102647& 8700/8870(6);8630(8)& 4.20&  SWP31145L&  3.79 &---&  2.17&  4.31\\
         &            &       & LWP21951L& 8.29 & & & \\
HD 103287& 9400/9360(8);9500(9)& 3.80&  SWP08198L& ---& ---&  1.26& --- \\
HD 116842& 7900/7931(3);8230(5)& 4.00&  SWP10283L&  1.79 & 1.32& --- & 1.00 \\
         &            &       & SWP10285L&  2.79 & 5.09& --- & 3.11 \\
         &            &       & SWP10285S&  3.11 & 3.24&  2.63 & 3.30 \\
HD 130109& 9475/9450(13)& 3.60&  SWP31552L&  5.55 &---& ---&  4.73 \\
         &            &       & LWP22392L& 6.60 & & & \\
         &            &       & LWP22507L& 5.22 & & & \\
HD 151676& 7750/---   & 3.95  & SWP33914L& ---& ---&  1.69& --- \\
HD 159561& 7900/7960(2);7923(4)& 3.70& SWP16490L&  4.77 &---& ---&  3.54\\
         &            &       & SWP16490S&  3.88 & 2.92 & ---& 2.92 \\
         &            &       &SWP17411L&  3.77 &---&  ---&  3.06 \\
         &            &       & SWP17411S&  3.63 & 2.73& ---&  2.77 \\
HD 159834& 8150/---   &       &  LWP21229L& 11.10 & & & \\
HD 187642& 7950/7800(13)& 4.10 & SWP45755L& ---& ---&  ---& ---\\
HD 203280& 7750/7825(13)& 3.80 & SWP45759L&  4.48 & 3.64 & 2.33 & 3.69\\
HD 214994& 9600/9680(12)& 3.65 & SWP43441L&  3.56 & 3.81 & 1.42&  4.15\\
HD 216956& 8800/8760(1) & 4.20 & LWP10680L& 9.00 & & & \\
         &              &      & LWP10681L& 12.75 & & & \\
         &              &      & SWP09134L& ---& ---& ---& ---\\
         &              &      & SWP09134S&  2.61 & 3.54& --- & 2.11\\
         &              &      & SWP09135S&  3.08 & 5.17& --- & 3.00 \\
HD 222661& 8300/---     & 4.15 & SWP15789S&  1.94 & 1.54 & 1.61& --- \\
\hline
\end{tabular}
\end{center}
\end{flushleft}
\footnotesize
{\bf Sources for T$_{eff}$:} {\bf 1:} Holweger \& Rentzsch-Holm (1995); 
{\bf 2:} Smalley \& Dworetsky (1995); {\bf 3:} Blackwell \& Lynas-Gray (1994); {\bf 4:} Alonso et al. (1996); 
{\bf 5:} Malagnini \& Morossi (1990); {\bf 6:} Smalley (1993); {\bf 7:}
Smalley \& Dworetsky (1993); {\bf 8:} Napiwotzki et al. (1993); {\bf 9:} 
Adelman et al. (1980); {\bf 10:} Nissen (1981); {\bf 11:} Van Veer-Menneret et al. 
(1989); {\bf 12:} Hill \& Landstreet (1993); {\bf 13:} Gerbaldi et al. 
(1989); {\bf 14:} Adelman (1978).
\end{table*}
\end{document}
