% Table 3 for paper ds7030 by Rossi C. et al. 
% accepted for pubblication in AA Supplement
\documentstyle {article}
%\pagestyle {empty}
\voffset=-4cm
%\hoffset=-2cm
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%\textheight=23cm
% 
\def\as{$\lceil$}
\def\ax{$\mid$} 
\def\az{$\lfloor$}
\def\sa{\noalign{\smallskip}}

\begin{document}
\setcounter {table}{2}
\begin{table*}
\caption[]{ 
The emission line spectrum of V380 Ori in January 1995 (OHP/AURELIE)
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 &~~~(1)   &  (2)~         &       &(3)&   & (4)     &~~(5) \\
\noalign{\smallskip}
\hline
\noalign{\medskip}
$\lceil $&4071.53 &  0.31 & 4071.007& NiII&  11 &   39& \\
$\lfloor$&4072.78 &  0.86 & 4072.561& CrII&  26 &   16& \\
\sa
$\lceil $&4161.88 &  0.29 & 4161.535& TiII&  21 &   25& \\
$\lfloor$&4164.05 &  0.94 & 4163.648& TiII& 105 &   29& \\
\sa
$\lceil $&4172.32 &  0.89 & 4171.910& TiII& 105 &   30& \\
$\mid   $&        &       & 4171.903& CrII&  18 &   30& contr \\
$\lfloor$&4173.78 & 1.93 & 4173.461& FeII&  27 &   23& p\\
\sa
$\lceil $&4177.52 &  0.88 & 4178.862& FeII&  28 &  -96& b\\ 
$\lfloor$&4179.29 & 2.33 & 4178.862& FeII&  28 &   31& p\\
\sa 
        &4227.04 &  0.54 & 4226.728& CaI &   2 &   22& \\
\sa
$\lceil $&4231.83 &  0.38 & 4233.172& FeII&  27 &  -95& b \\
$\lfloor$&4233.60 & 4.90 & 4233.172& FeII&  27 &   30& p\\
\sa
$\lceil $&4243.25 &  0.61  & 4242.38 & CrII & 31 &     & blend\\  
\ax     &        &       & 4242.886& VII & 200 &     & id?\\
$\lfloor$&        &       & 4244.90 & [FeII]&21F&     & in red wing \\
\sa
        &4247.05 & 1.02   & 4246.822& ScII&   7 &   16& \\
\sa
$\lceil $&4257.96 &  0.13 & 4258.154& FeII&  28 &  -14& b\\
$\mid   $&4258.83 &  0.42 & 4258.154& FeII&  28 &   48& p\\
$\mid   $&4261.47 &  0.42 & 4260.763& VII &  18 &   50& \\
$\lfloor$&4263.18 &  0.28 & 4263.134& TiI & 162 &    3& \\
\sa
$\lceil $&4272.42 &  0.83 & 4273.326& FeII&  27 &  -64& b\\
$\mid   $&4274.37 &  0.48 & 4273.326& FeII&  27 &   73& p\\
$\lfloor$&4277.77 &  0.33 & 4276.830& [FeII]&21F&   66& \\
\sa
$\lceil $&4288.03 &  0.29 & 4287.400& [FeII]& 7F&    44  & \\
$\lfloor$&4290.66 & 1.57 & 4290.219& TiII&  41 &   31& \\
\sa
$\lceil $&4294.21 &  0.82 & 4294.099& TiII&  20 &    8& \\
$\mid   $&4295.64 &  0.73 & 4294.767& ScII&  15 &   61& \\
$\lfloor$&4297.31 &  1.08 & 4296.572& FeII&  28 &   52& p\\
$\lceil $&4300.29 & 1.72 & 4300.049& TiII&  41 &   17& \\
$\mid   $&4302.36 & 1.49 & 4301.914& TiII&  41 &   31& \\
$\lfloor$&4303.62 & 1.65 & 4303.176& FeII&  27 &   31& p\\
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
\end{table*}
\vfill\eject

\setcounter {table}{2}
\begin{table*}
\caption[]{ 
(continued)  The optical spectrum of V380 Ori in January 1995 
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 &  ~~(1)   &  (2)~         &       &(3)&   & (4)     &~~(5) \\
\noalign {\smallskip}
\hline
\noalign{\medskip}
\as &4308.35 & 1.06 & 4307.863& TiII&  41 &   34& \\
\ax &4313.35 & 0.82 &  4312.864& TiII&  41 &    34 & \\
\ax &4314.57 & 0.70 &  4314.083& ScII&  15 &    34 & \\
\ax &4315.34 & 0.75 &  4314.975& TiII&  41 &    25 & \\ 
\az &        &      &  4314.979& FeII&   k &    25 & contr\\
\sa
    &4352.08 & 3.51 &  4351.769& FeII&  27 &    21 & p\\
\sa
\as &4357.70 & 0.22 &  4357.584& FeII&   k &     8 & \\
\ax &4358.52 & 0.31 &  4358.370& [FeII]&21F&     10 &\\
\az &4359.50 & 0.16 &  4359.340& [FeII]& 7F&     11 &\\
\sa
    &4367.55 & 0.27 &  4367.659& TiII& 104 &   -8 & contr\\
    &        &      &  4368.107& CrII&  37 &   63 & contr\\
\sa
    &4375.25 & 0.64 &  4374.457& ScII&  14 &   55 & \\
\sa
\as &4383.24 & 0.26 &  4382.750& [FeII]& 6F&   34 & contr\\
\ax &4384.06 & 0.96 &  4385.387& FeII&  27 &  -91 & b\\
\ax &4385.79 & 1.82 &  4385.387& FeII&  27 &   28 & p\\
\az &4387.35 & 0.31 &  4386.844& TiII& 104 &   35 & \\
\sa
    &4390.62 & 0.24 &  4390.14 & NaI &  17 &      & \\
    &        &      &  4390.585& MgII&  10 &      & contr \\
\sa
\as &4394.45 & 0.70 &  4394.051& TiII&  51 &   27 & \\
\ax &4395.45 & 1.21 &  4395.033& TiII&  19 &   29 & \\
\az &4396.25 & 0.49 &  4395.850& TiII&  61 &   27 & \\
\sa
    &4400.11 & 1.18 &  4399.772& TiII&  51 &   23 &\\
\sa
    &4404.91 & 0.27 &  4404.750& FeI &  41 &   11 &\\
\sa
\as &4410.25 & 0.17 &  4409.516& TiII&  61 &   50 &\\
\az &4411.53 & 0.32 &  4411.074& TiII& 115 &   31 &\\
\sa
\as &4415.64 & 0.99 &  4416.830& FeII&  27 &  -81 & b\\
\ax &        &      &  4413.78 & [FeII]& 7F&      & contr \\
\ax &4417.25 & 1.84 &  4416.830& FeII&  27 &   29 & p\\
\ax &        &      &  4416.27 & [FeII]& 6F&      & contr\\
\ax &4418.25 & 0.45 &  4417.719& TiII&  40 &   36 & \\
\az &4418.90 & 0.46 &  4418.330& TiII&  51 &   39 & \\
\sa
\as &4442.62 & 0.29 &  4441.734& TiII&  40 &   60 & \\
\ax &4444.10 & 1.16 &  4443.794& TiII & 19 &   21 & \\
\az &4445.08 & 0.47 &  4444.558& TiII&  31 &   35 & \\
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
\end{table*}
\vfill\eject

\setcounter {table}{2}
\begin{table*}
\caption[]{ 
(continued)  The optical spectrum of V380 Ori in January 1995 
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 &  ~~(1)   &  (2)~         &       &(3)&   & (4)     &~~(5) \\
\noalign {\smallskip}
\hline
\noalign{\medskip}
    &4450.92 & 0.77 &  4450.482& TiII&  19 &   30 & \\
    &        &      &  4452.110& [FeII]& 7F&   44 & contr\\
\sa
\as &4468.63 & 1.36&  4468.507& TiII&  31 &    8 & \\
\ax &4469.60 & 0.36 &  4469.138& TiII&  18 &   31 & \\
\ax &4470.76 & 0.21 &  4470.857& TiII&  40 &   -7 & \\
\az &        &      &  4471.477& HeI &     &      & contr \\
\sa
\as  &4481.7 &  1.00 &  4481.330& MgII&   4 &   & \\
\az  &4481.96 &   &  4481.330& MgII&   4 & 42  & \\
\sa
\as &4487.70 & 0.44 &  4489.183& FeII&  37 &  -99 & b\\
\ax &4489.69 & 1.60 &  4489.183& FeII&  37 &   34 & p\\
\az &4491.85 & 1.92 &  4491.405& FeII&  37 &   30 & p\\
\sa
\as &4499.92 & 0.40 &  4501.273& TiII&  31 &  -90 & b id? \\
\az &4501.81 & 1.49 &  4501.273& TiII&  31 &   36 & \\
\sa
\as &4507.04 & 0.64 &  4508.288& FeII&  38 &  -83 & b\\
\ax &4508.76 & 2.69 &  4508.288& FeII&  38 &   31 & p\\
\az &4510.56 & 0.43 &  4509.610& [FeII]& 6F&   63 & ? \\
\sa
\as &4513.88 & 0.45 &  4515.339& FeII&  37 &  -97 & b\\
\ax &4515.88 & 2.71 &  4515.339& FeII&  37 &   36 & p\\
\ax &4518.90 & 0.77 &  4520.224& FeII&  37 &  -88 & b\\
\ax &4520.94 & 2.55 &  4520.224& FeII&  37 &   48 & p\\
\az &4523.15 & 3.50 &  4522.634& FeII&  38 &   34 & p\\
\sa
    &4529.75 & 0.66 &  4529.474& TiII&  82 &   18 & \\
\sa
\as &4532.66 & 0.42 &  4534.168& FeII&  37 & -100 & b\\
\az &4534.53 & 1.66 &  4534.168& FeII&  37 &   24 & p\\
\sa
\as &4540.03 & 0.31 &  4541.524& FeII&  38 &  -99 & b\\
\ax &4541.97 & 0.96 &  4541.524& FeII&  38 &   30 & p\\
\az &4543.36 & 0.36 &  4542.807& CrII&  16 &   37 & \\
\sa
\as &4548.12 & 1.16 &  4549.474& FeII&  38 &  -89 & b\\
\ax &4549.93 & 2.82 &  4549.474& FeII&  38 &   30 & p\\
\az &4550.52 & 1.66 &  4549.617& TiII&  82 &   60 & \\
\sa
\as &4554.33 & 0.89 & 4555.893& FeII & 37 & -103 & b\\
\ax &4556.50 & 2.96 & 4555.893& FeII & 37 &   40 & p\\
\az &4558.99 & 2.01 & 4558.650& CrII & 44 &   22 &  \\
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
\end{table*}
\vfill\eject

\setcounter {table}{2}
\begin{table*}
\caption[]{ 
(continued)  The optical spectrum of V380 Ori in January 1995 
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 &   ~~(1)   &  (2)~         &       &(3)&   & (4)     &~~(5) \\
\noalign {\smallskip}
\hline
\noalign{\medskip}
\as &4562.22 & 0.29 & 4563.761& TiII & 50 & -101 & \\
\az &4564.32 & 1.40 & 4563.761& TiII & 50 &   37 & \\
\as &4570.40 &   0.36 & 4571.968& TiII & 82 & -103 & \\
\ax &4572.48 &   1.98 & 4571.968& TiII & 82 &   34 & \\
\ax &4574.91 &   0.41 & 4576.340& FeII & 38 &  -94 & b\\
\az &4576.91 &   1.39 & 4576.340& FeII & 38 &   37 & p\\
\sa
\as &4582.18 &   1.49 & 4583.837& FeII & 38 & -108 & b\\
\ax &        &        & 4582.835& FeII & 26 &      & contr\\
\az &4584.31 &   5.21 & 4583.837& FeII & 38 &   31 & p\\
\sa
    &4588.84 &   1.76 & 4588.199& CrII & 44 &   42 &\\
\sa
\as &4617.16 &   0.49 & 4616.629& CrII & 44 &   35 &  \\
\ax &4619.20 &   1.19 & 4618.803& CrII & 44 &   27 &  \\
\az &4621.06 &   0.75 & 4620.521& FeII & 38 &   35 & p\\
\sa
\as &4627.83 &   0.67 & 4629.339& FeII & 37 &  -98 & b\\
\az &4629.91 &   3.30 & 4629.339& FeII & 37 &   37 & p\\
\sa
\as &4634.49 &  1.08  & 4634.070& CrII & 44 &   27 & \\
\az &4636.73 &  0.36 & 4636.320& TiII & 38 &   27 & \\
\sa
    &4657.83 &  0.52 & 4657.206& TiII & 59 &   40 & \\
\sa
\as &4665.33 &  0.24 & 4666.758& FeII & 37 &  -92 & b\\
\az &4667.23 &  0.69 & 4666.758& FeII & 37 &   30 & p\\
\sa
    &4670.73 &  0.43 & 4670.407& ScII & 24 &   21 &\\
\sa
\as &4730.05 &  0.13 & 4731.453& FeII & 43 &  -89 & b\\
\az &4732.06 &  1.02 & 4731.453& FeII & 43 &   39 & p\\
\sa
    &4764.43 &  0.35 & 4763.881& TiII & 48 &   34 & \\
\sa
    &4780.47 &  0.45  & 4779.985& TiII & 92 &   30 & \\
\sa

\as &4803.40 &  0.31 & 4803.019& ScII &    &   24 & id?\\ 
\az &4805.66 &  0.57 & 4805.085& TiII & 92 &   36 &\\
\sa
    &4811.57 &  0.17 & 4810.745& FeII &169 &   51 &\\  
\sa
    &4815.05 &  0.08 & 4814.550& [FeII] & 20F&   31 &\\
\sa
\as &4822.68 &  0.17 & 4824.100& CrII & 30 &  -88 & b id?\\  
\az &4824.72 & 1.10 & 4824.100& CrII & 30 &   39 & \\
\sa
\as &4874.58 & 0.31 & 4874.014& TiII &114 &   35 &\\
\az &4876.95 & 0.63 & 4876.399& CrII & 30 &   34 &\\
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
\end{table*}
\vfill\eject

\setcounter {table}{2}
\begin{table*}
\caption[]{ 
(continued)  The optical spectrum of V380 Ori in January 1995 
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 &  ~~(1)   &  (2)~         &       &(3)&   & (4)     &~~(5) \\
\noalign {\smallskip}
\hline
\noalign{\medskip}
\as &4920.54 & -0.30 & 4923.927& FeII & 42 & -206 & pcy\\ 
\az &4924.62 &  12.68 & 4923.927& FeII & 42 &   42 & p\\
\sa
    &4994.13 & 1.11 & 4993.358& FeII & 36 &   46 & p\\
\as &5014.76 & -0.30 & 5018.440& FeII & 42 & -220 & pcy\\
\az &5019.17 & 15.06 & 5018.440& FeII & 42 &   44 & p\\
\sa
\as &5128.18 &  0.55 & 5127.866& FeII &167 &      & \\
\ax &        &        & 5127.652& NiII &    &   31 & contr\\
\az &5130.31 &  0.95 & 5129.750& FeII &  k &   33 &\\
\sa
\as &5165.31 & -0.52 & 5169.033& FeII & 42 & -216 & pcy\\  
\az &5169.71 & 18.11 & 5169.033& FeII & 42 &   39 & p\\
\sa
    &5173.64 & 1.64 & 5172.990& FeII &185 &   38 &    \\
\sa
    &5184.73 & 3.25 & 5183.604& MgI  &  2 &   65 &\\
\sa
    &5195.86 & 0.41 & 5197.577& FeII & 49 &  -99 & b\\
\sa
    &5198.34 & 6.17 & 5197.577& FeII & 49 &   44 & p\\
\sa
    &5227.57 & 1.15 & 5226.543& TiII & 70 &   59 & \\
\sa
\as &5232.95 & 0.70 & 5234.625& FeII & 49 &  -96 & b\\
\ax &5235.44 & 0.65 & 5234.625& FeII & 49 &   47 & p\\
\az &5237.95 & 1.25 & 5237.329& CrII & 43 &   36 &\\
\sa
    &5254.54 & 0.33 & 5254.467& TiI  &     &   4 & id?\\
\sa
    &5265.88 & 0.93 & 5264.812& FeII & 48 &   61 & p\\
\sa
\as &5270.79 & 0.87 & 5270.027& FeII &  k &   43 & \\
\ax &5273.94 & 0.19 & 5273.380& [FeII]&18F&   32 &\\
\ax &5274.53 & 0.77 & 5276.002& FeII & 49 &  -84 & b\\
\az &5276.77 & 7.45 & 5276.002& FeII & 49 &   44 & p\\
\sa
\as &5280.15 & 0.49 & 5279.876& CrII & 43 &   16 & \\
\ax &5282.66 & 0.27 & 5284.109& FeII & 41 &  -82 & b\\
\az &5285.04 & 2.80 & 5284.109& FeII & 41 &   53 & p\\
\sa
\as &5314.80 & 1.26 & 5316.615& FeII & 49 & -102 & b\\
\az &5317.47 & 11.79 & 5316.615& FeII & 49 &   48 & p\\
\sa
    &5326.51 & 1.72 & 5325.553& FeII & 49 &   54 & p\\
%
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
\end{table*}
\vfill\eject

\setcounter {table}{2}
\begin{table*}
\caption[]{ 
(continued)  The optical spectrum of V380 Ori in January 1995 
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 &  (1)   &  (2)         &       &(3)&   & (4)     &~~(5) \\
\noalign {\smallskip}
\hline
\noalign{\medskip}
    &5337.67 & 1.33 & 5336.809& TiII & 69 &      &  \\
    &        &      & 5336.717& NiII &    &   54 & contr\\
\sa
\as &5361.00 & 0.21 & 5362.869& FeII & 48 & -105 & b\\
\az &5363.56 & 3.41 & 5362.869& FeII & 48 &   39 & p\\
\sa
    &5366.18 & 0.18 & 5365.550& FeII &  k &   35 &  \\
\sa              
    &5381.77 & 0.44 & 5381.015& TiII & 69 &   42 & \\
\sa
    &5414.23 & 0.70 & 5414.073& FeII & 48 &    9 & p\\
\sa
\as &5426.03 &  1.38 & 5425.257& FeII & 49 &   43 & p\\
\ax &5428.64 &  0.34 & 5427.826& FeII &  k &   45 &\\
\ax &5431.98 &  0.46 & 5431.539& FeII &  k &   24 &\\
\az &5433.92 &  0.27 & 5433.150& [FeII] & 18F &  43 & contr\\
\sa
    &5460.73 & 0.31 & 5460.469& TiI  &  3 &   14 & \\
\sa
\as &5477.88 &      & 5477.45 & CrII & 50 &      &\\
\az &5479.18 &  0.25 & 5478.365& CrII & 50 &   45 &\\
\sa
\as &5527.70 & 0.65 & 5526.790& ScII & 31 &   49 &\\
\az &5529.69 & 0.52 & 5529.932& FeII &224 &  -13 &\\
\sa
    &5535.58 & 3.02 & 5534.847& FeII & 55 &   40 &  \\ 
\sa
    &5658.58 & 0.57 & 5657.896& ScII & 29 &   36 &\\
\sa
    &5684.81 & 0.23 & 5684.202& ScII & 29 &   32 &\\
\sa
\as &5875.16 & 2.30 & 5875.630& HeI  & 11 & -23 &\\
\az &5876.56 & -0.1 & 5875.630& HeI  &  11 &  48 & ca\\ 
\as &5888.15 & 0.47 & 5889.950& NaI  &  1 &  -92 & b\\
\ax &5890.45 &     & 5889.950& NaI  &  1 &   25 & is\\ 
\ax &5890.67 & 3.23 & 5889.950& NaI  &  1 &   37 & \\
\ax &5896.40 &     & 5895.920& NaI  &  1 &   25 & is\\
\ax &5896.64 & 3.53 & 5895.920& NaI  &  1 &   36 & \\
\az &5989.43 & 0.22 &         &      &    &      & id?\\
\sa
    &5992.22 & 1.50 & 5991.376& FeII & 46 &   42 & p\\
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
\end{table*}
\vfill\eject

\setcounter {table}{2}
\begin{table*}
\caption[]{ 
(continued)  The optical spectrum of V380 Ori in January 1995 
}  
\begin{flushleft}
\begin{tabular}{llrllrrl}
\hline
\noalign{\smallskip} 
 &obs.wl. &F$^o$/W$_{eq}$&lab.wl.&ion&RMT&V$_{rad}$&remarks \\ 
 & ~~(1)  &  (2)~        &       &(3)&   & (4)     &~~(5) \\
\noalign {\smallskip}
\hline
\noalign{\medskip}
    &6085.04 & 0.90 & 6084.111& FeII & 46 &   46 & p\\
\sa
\as &6146.43 & 0.71 & 6149.258& FeII & 74 & -138 & b\\
\az &6149.39 & 3.87 & 6149.258& FeII & 74 &    7 & p\\
\sa
\as &6236.61 & 0.50 & 6238.392& FeII & 74 &  -86 & b\\
\az &6239.39 & 2.93 & 6238.392& FeII & 74  &  48 & p\\
\sa
\as &6245.42 & 0.53 & 6247.557& FeII & 74 & -103 & b\\
\az &6248.44 & 4.82 & 6247.557& FeII & 74 &   42 & p\\
\sa
    &6300.66 & 0.65 & 6300.23 & [OI] & 1F &   22 & \\
\sa
    &6318.57 &  1.14 & 6317.983& FeII &  k &   28 &\\
\sa
    &6346.41 & 3.03 & 6345.435& FeII &  k &   46 &\\
\sa
\as &6364.38 & 0.26 & 6363.88 & [OI] &  1F&  24 & \\  
\ax &6367.52 & 0.43 & 6369.462& FeII & 40 &  -92 & b id?\\
\az &6370.40 & 2.18 & 6369.462& FeII & 40 &   44 & p\\
\sa
    &6383.99 & 0.82 & 6383.753& FeII &    &      & id?\\ 
\sa
    &6386.22 & 0.39 & 6385.451& FeII &  k &   36 &\\
\sa
\as &6414.90 & 0.34 & 6416.919& FeII & 74 &  -94 & b\\
\az &6417.86 & 2.31 & 6416.919& FeII & 74 &   44 & p\\
\sa
\as &6454.41 & 0.87 & 6456.383& FeII & 74 &  -92 & b\\
\az &6457.29 & 6.76 & 6456.383& FeII & 74 &   42 & p\\
\sa
    &6482.83 & 0.97 & 6482.204& FeII &199 &   29 &\\
\sa
    &6492.84 & 1.18 & 6491.562& TiII & 91 &   59 &\\
\sa
\as &6513.76 & 0.66 & 6516.080& FeII & 40 & -107 & b id?\\
\az &6517.12 & 4.63 & 6516.080& FeII & 40 &   48 &  \\
\noalign{\medskip}
\hline 
\noalign {\medskip}
\end{tabular}
%\medskip\noindent
\end{flushleft} 
%
{\it Notes to the table:}
The hydrogen Balmer lines are not included in this table;
$^1$ Heliocentric wavelength (in \AA). 
$^2$ Line intensity: Positive values: integrated emission line flux 
(in 10$^{-13}$ erg cm$^{-2}$ s$^{-1}$ \AA$^{-1}$) ~~ 
Negative values: absorption line equivalent width.  
$^3$ Line identification: laboratory wavelength (in \AA), 
    ion of the contributor and Moore's multiplet number; k: Kurucz table
$^4$ Radial velocity (heliocentric in km s$^{-1}$). 
$^5$ Remarks: p: principal component; b: blue shifted component;
    pcy: P Cygni absorption component;
    ca: narrow central/shell absorption;
    is: interstellar absorption line;
    contr: minor contributor to the line; id?: uncertain identification.  
\end{table*}
%
\end{document}
