\documentstyle{l-aa}

\begin{document}
\thesaurus{06(08.02.5; 08.06.3; 08.08.1; 08.03.4)}
\title{Spectrophotometric study of southern symbiotic stars}
\author{J. Miko{\l}ajewska \inst{1}
  \and A. Acker \inst{2}
  \and B. Stenholm \inst{3}}
\institute{Copernicus Astronomical Center, Bartycka 18, PL--00716 Warsaw, Poland (mikolaj@camk.edu.pl)
    \and URA 1280, Observatoire de Strasbourg, 11 rue de l'Universit\'{e},
F--67000 Strasbourg, France
    \and Lund Observatory, Box 43, S--22100 Lund, Sweden}
\offprints{J. Miko{\l}ajewska}
\date{}
\maketitle

\begin{abstract}
We have analyzed the optical spectra of 67 symbiotic stars
and objects suspected of being symbiotic,
and found 18 new symbiotic systems.
This is the largest homogeneous set of optical
spectrophotometric data for symbiotic binaries
ever studied. We have derived the reddenings and distances
for all systems, estimated the IR classes (S and D)
for the new systems,
and determined the location of the hot components 
in the Hertzsprung-Russell diagram. 

\keywords{Binaries: symbiotic -- stars: fundamental parameters --
Hertzsprung-Russell diagram -- circumstellar matter}

\end{abstract}


\begin{table*}
\caption[]{Emission line fluxes in units of 
$10^{-13} \rm erg cm^{-2} s{-1}$}
\begin{flushleft}
\scriptsize
\begin{tabular}{l c c c c c c c c c c c c c c c c}
\noalign{\smallskip}
\hline
\noalign{\smallskip}
\multicolumn{1}{l}{Star} & \multicolumn{1}{c}{JD} & 
\multicolumn{4}{c}{H\,I} & \multicolumn{3}{c}{[O\,III]}
& \multicolumn{3}{c}{He\,I} & \multicolumn{2}{c}{He\,II}
& \multicolumn{1}{c}{O\,VI} & \multicolumn{2}{c}{[Fe\,VII]} \\
   & 244... & 6563 & 4860 & 4340 & 4100 & 4363 & 4960 & 5007
   & 5876 & 6678 & 7065 & 4686 & 5412 & 6825 & 5721 & 6086 \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
He2--38 & 5821 & 518.8 & 17.3 & 5.00 & 2.43 & 9.36 & 12.8 & 44.9 & 7.54 & 3.55 & 8.93 & 5.71 & 1.04 & 13.8 & 1.31 & 2.67 \\
He2-87 & 5817 & 3.56 & 0.05 & & & & & & 0.09 & 0.05 & 0.14 & & & 0.06 & & \\
St2--22 & 8067 & 11.6 & 0.63 & 0.15 & & & 0.08 & 0.20 & 0.35 & 0.38 & 0.50 & 0.31 \\
V704 Cen & 5818 & 7.20 & 0.58 & & & 0.25 & 0.29 & 0.88 & 0.31 & 0.16 & 0.43 & \\
V852~Cen & 5457 & 173.4 & 10.3 & & & & 11.2 & 36.7 & 4.77 & 1.20 & & 1.54 & 0.31 & \\
     & 6263 & 330.2 & 33.5 & 12.0 & 6.72 & 12.3 & 32.3 & 97.3 & 9.57 & 2.83 & 10.3 & 5.95 & 1.52 & \\
     & 6280 & 142.7 & 13.3 & 5.08 & 2.83 & 5.57 & 13.6 & 38.7 & 4.33 & 1.37 & 4.53 & 2.34 & 0.45 & \\
V835 Cen & 5817 & 411.4 & 13.5 & 3.81 & 1.52 & 6.20 & 20.0 & 66.3 & 4.47 & 2.88 & 7.41 & 3.98 & 1.06 & 26.6 & 1.30 & 2.72 \\
He2--127 & 5817 & 88.8 & 4.70 & 1.34 & & 0.60 & 1.24 & 4.72 & 1.07 & 0.70 & 1.46 & 2.41 & 0.29 & 5.46 & 0.46 & 0.86 \\
Hen 1092 & 5817 & 31.1 & 4.00 & 1.63 & 0.67 & 0.45 & & & 0.95 & 0.50 & 1.13 & 3.70 & 0.35 & 2.53 & 0.43 & 0.78 \\
HD 330036 & 5818 & 110.7 & 18.2 & 7.90 & & 26.2 & 73.8 & 216.0 & 9.16 & 1.82 & 7.64 & 2.25 & \\
He2--147 & 5458 & 2.48 & 0.34 & 0.14: & & 0.25 & 1.32 & 4.25 & 0.11 & 0.05: & 0.08 & 0.03: & \\
	 & 8066 & 3.39 & 0.43 & & & 0.23 & 1.77 & 5.62 & 0.14 & 0.06: & 0.10 & 0.03: & \\
He2--156  & 5817 & 60.4 & 4.95 & 1.50 & & & & & 1.09 & 0.59 & 0.66 & \\
He2--171 & 5819 & 47.6 & 3.59 & 0.94 & 0.37 & 1.12 & 3.52 & 12.6 & 0.69 & 0.36 & 0.85 & 2.14 & 0.31 & 0.95 & 1.22 & 2.49 \\
He2--173 & 5817 & 65.2 & 3.14 & 0.82 & & 0.77 & 0.80 & 3.13 & 2.29 & 2.36 & 2.86 & 0.96 & 0.12 & & \\
He2--176 & 5457 & 42.8 & 0.38 & & & & 0.07 & 0.18 & 0.57 & 0.93 & 2.20 & 0.19 & 0.06 & 1.02 & \\
KX TrA & 5819 & 454.1 & 37.9 & 11.1 & 6.01 & 4.27 & 4.96 & 15.0 & 6.66 & 7.61 & 8.46 & 29.3 & 3.18 & 21.0 & 4.95 & 9.03 \\
MaC 1--3 & 7675 & 8.05 & 0.28 & & & & & & 0.12 & 0.08 & 0.16 & 0.09 & & 0.28 & 0.05 & 0.12 \\
V455 Sco & 5820 & 172.9 & 7.17 & 1.66 & 0.99 & 0.57 & 0.84 & 2.63 & 3.25 & 1.57 & 4.21 & 6.99 & 1.04 & 6.69 & 2.26 & 4.13 \\
AS 221 & 5817 & 18.2 & 0.74 & 0.22 & & 0.16 & 0.07 & 0.37 & 0.51 & 0.49 & 0.97 & 0.67 & 0.10 & 0.21 & 0.24 & 0.49 \\
H2--5 & 5820 & 6.80 & 0.38 & & & & & & 0.17 & 0.07 & 0.16 & 0.23 & 0.03 & 0.66 & & 0.08 \\
Th3--7 & 6622 & 8.52 & 0.59 & & & & & & 0.25 & 0.33 & & & & 0.31 & 0.31 & 0.36 \\
Th3--17 & 6265 & 4.96 & 0.16 & & & & & 0.08 & 0.12 & 0.24 & 0.20 & \\
Th3--18 & 5820 & 20.3 & 0.67 & 0.13 & & & & & 0.22 & 0.36 & 0.37 & 0.29 & 0.04 & 1.42 & \\
Th3--20 & 5821 & 7.43 & 0.28 & 0.05 & & 0.06 & 0.22 & 0.19 & 0.15 & 0.37 & 0.20 & 0.09 & 0.26 & 0.10 & 0.15 \\
Th3--29 & 6262 & 8.34 & 0.18 & & & & & 0.08 & 0.18 & 0.24 & 0.24 & & & 0.06 & \\
Th3--30 & 6262 & 8.62 & 0.21 & & & & & & 0.14 & 0.25 & 0.22 & 0.09 & 0.01 & 0.37 & \\
Th3--31 & 5821 & 4.17 & 0.14 & & & & & 0.09 & 0.13 & 0.25 & 0.28 & & \\
M1--21 & 5818 & 153.0 & 16.4 & 4.86 & 2.53 & & & 1.26 & 4.02 & 2.68 & 4.14 & 7.53 & 0.75 & 5.63 & 0.60 & 0.87 \\
He2--251 & 5821 & 10.9 & 0.19 & & & & & 0.12 & 0.10 & 0.05 & 0.18 & & & 0.42 & \\
W16--296  & 8066 & 14.4 & 0.46 &   & &  &   & 0.09 & 0.50 & 0.55 & 0.81 &   &    \\
WR 99 & 8066 & 49.3 & 0.97 & 0.14 & & & 0.18 & 0.63 & 1.13 & 1.34 & 2.87 & 0.18 & 0.06 & 0.64 & 0.06 & 0.15 \\
AE Ara & 5821 & 182.1 & 27.4 & 10.0 & 7.14 & 3.02 & 6.43 & 19.1 & 4.99 & 3.43 & 5.50 & 2.49 & \\
UU Ser & 5819 & 43.7 & 4.48 & 1.21 & 0.54 & 0.09 & & 0.43 & 1.06 & 1.27 & 1.35 & 4.26 & 0.40 & 3.26 & 0.19 & 0.30 \\
AS 241 & 6266 & 3.63 & 0.30 & & & & & & 0.05 & 0.08 & 0.09 & \\
He2--275 & 6281 & 7.85 & 0.71 & 0.27: & & & & & 0.24 & 0.32 & 0.33 & 0.24 & & 0.71 & \\
HD 316285 & 6281 & 1462 & 146.2 & 31.4 & 10.6 & 10.7 & & & 77.3 & 70.6 & 158.2 & \\
V4141 Sqr & 5821 & 12.1 & 0.93 & 0.29 & & & 0.15 & 0.55 & 0.38 & 0.16 & 0.54 & \\
ALS 2 & 5817 & 19.6  & 1.95 & 0.77 & 0.25 & & & & 0.76 & 0.78 & 1.10 & 1.05 & 0.14 & 1.38: \\
AS 245  & 5818 & 10.5 & 0.26 & &  &   & 0.11 & 0.42 & 0.20 & 0.20 & 0.54 & 0.18 & 0.04 & 0.78 & 0.16 & 0.32 \\
He2--294 & 5821 & 11.5 & 0.39 & & & & & & 0.27 & 0.20 & 0.33 & 0.23 & &  1.13 & & \\
Bl3--6 & 6266 & 2.82 & 0.11 & & & & & & 0.05 & 0.09 & 0.10 & 0.08 & & 0.35 & \\
MaC 1--9 & 7676 & 10.6 & 0.82 & 0.27 &  & 0.07 & & 0.18 & 0.44 & 0.77 & 0.70 & 0.05 &   \\
V2416 Sgr & 5821 & 93.9 & 2.12 & 0.32 & & & & & 1.11 & 1.04 & 1.94 & 1.13 & 0.20 & 2.54 & 0.48 & 0.93 \\
AS 269 & 6278 & 107.6 & 3.23 & & & & & & 0.56 & 0.45: & 0.49 & \\
Ap1--8 & 5458 & 20.2 & 1.27 & 0.54 & & 0.09 & & 0.46 & 0.72 & 0.53 & 0.86 & 1.02 & & 0.51: & 0.18 & 0.34 \\
SS 122   & 7676 & 126.1 & 11.0 & 2.77 & 1.38 & 0.94 & 1.91 & 8.04 & 5.24 & 3.00 & 7.13 & 3.14 & 0.63 & 1.12 & 2.50 & 4.70 \\
H2--38 & 5458 & 179.7 & 9.20 & 2.50 & 0.94 & 5.18 & 10.4 & 33.7 & 2.37 & 0.94 & 3.14 & 4.78 & 0.65 & 14.2 & 1.03 & 2.17 \\
SS 129   & 8067 & 6.11 & 0.39 &   &  & &   &   & 0.86 & 0.33 & 0.82 & 0.61 &   & 0.90 \\
V615 Sgr & 6278 & 140.1 & 25.7 & 9.63 & 5.30 & 1.58 & & 2.66 & 4.93 & 6.86 & 5.22 & 0.44 & \\
AS 280 & 6278 & 33.5 & 10.0 & 5.55 & 2.64 & & & 0.65 & 3.03 & 1.80 & 1.52 & 6.89 & & \\
Ap1--9   & 6278 & 58.7 & 5.24 & 1.33 &  & &  & 0.67 & 2.20 & 2.12 & 2.27 & 0.17 & \\
AS 281   & 6278 & 134.0 & 11.0 & 4.00 & 1.77 &  &   &   & 1.94 & 1.43 & 2.33 & 7.00 & 0.85 & 5.76 & 0.60 & 0.89 \\
V2506 Sgr & 5816 & 55.9  & 5.86 & 1.94 & &   &   &   & 0.92 & 0.85 & 1.03 & 2.83 & 0.30 & 2.87 & 0.14 & 0.45 \\
V2756 Sgr & 6280 & 37.3 & 5.30 & 2.14 &  & 0.76 & 1.48 & 4.45 & 2.17 & 1.32 & 1.75 & 4.00 & 0.25: & \\
HD 319167 & 6280 & 115.9 & 13.8 & 4.17 &  & 3.01 & 1.42 & 5.30 & 5.60 & 3.71 & 6.29 & 1.36 & \\
He2--374 & 6280 & 48.6 & 2.28 & 0.53 & & 0.44 & 0.33 & 1.22 & 1.82 & 1.56 & 3.29 & 0.57 & \\
He2--376 & 6267 & 18.7 & 1.91 & &   &   &   & 0.84 & 1.00 & 0.72 & 0.91 &   & \\
AS 299   & 8067 & 107.6 & 15.1 & 4.15 & 1.89 &  &   & 1.49 & 5.48 & 4.83 & 5.91 & 0.74 & \\
V2601 Sgr & 5816 & 3.66 & 0.35 & 0.15: & & 0.15: & & 0.10: & 0.03: & 0.09: & 0.09: & 0.03: & \\
K 3--9 & 6265 & 12.3 & 0.24 & & & & 0.12 & 0.59 & 0.21 & 0.11 & 0.34 & 0.13 & & 0.24 & 0.25 & 0.60 \\
AS 316 & 6274 & 105.0 & 7.18 & 1.75 & 0.57 &  & & & 0.78 & 0.90 & 1.03 & 4.73 & 0.56 & 8.68 \\
AS 323 & 6280 & 19.8 & 1.49 & 0.65 & & & & & 0.41 & 0.53 & 0.56 & 1.51 & 0.19 & 0.90 & 0.12 & 0.20 \\
AS 327 & 8067 & 96.6 & 9.90 & 2.91 & 1.27 & & & & 2.99 & 3.18 & 3.87 & 4.65 & 0.74 & 6.53 \\
Pe2--16 & 5819 & 15.1 & 0.54 & & & & 0.06 & 0.14 & 0.53 & 0.50 & 1.08 & 0.30 & & 0.06 & 0.06 & 0.13 \\
V1413~Aql & 7677 & 58.3 & 7.78 & 2.55 & 1.20 & 0.26 & 0.53 & 1.89 & 3.90 & 1.92 & 2.27 & \\
MaC 1--17 & 8067 & 8.00 & 0.78 & 0.21 & & 0.09 & & & 0.34 & 0.73 & 0.42 & 0.17 & 0.02 & \\
V352 Aql & 7679 & 5.53 & 0.41 & 0.12 & & & & & 0.08 & 0.10 & 0.11 & 0.29 & 0.04 & 0.56 & 0.02: & 0.08 \\
ALS 1 & 5819 & 14.3 & 1.93 & 0.66 & & & & & 0.64 & 0.77 & 0.78 & 0.21 & 0.02: & 0.15: \\
\noalign{\smallskip}
\hline
\end{tabular}
\end{flushleft}
\end{table*}

\setcounter{table}{2}
\begin{table*}
\caption[]{Reddening estimates}
\begin{flushleft}
\scriptsize
\begin{tabular}{l c c c c c c c c} 
\noalign{\smallskip}
\hline
\noalign{\smallskip}
\multicolumn{1}{l}{Star} & \multicolumn{1}{c}{Type}
& \multicolumn{7}{c}{E(B--V)}\\
  &   & H~I (case B) & H~I ($\tau_{\rm H\alpha}$) 
  & He I & He II & [Fe~VII] & IR & Adopted \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
He2--38   & D & & 1.6 ($\sim 10$) & 1.6 & 1.5 & 1.5 & 2.5: & 1.5 \\
He2--87   & S & 3.0 & 1.8 $\div$ 2.5 & 1.0: & & & 2.0 & 2.0 \\
St2--22   & S &  & 1.4 ($\sim 10$) & 1.0 & & & & 1.0 \\
V704 Cen  & D & 1.3 &  & 1.8 & & & & 1.5 \\
V852~Cen  & D & & 0.8 ($\sim 10$) & 0.5 & 1.7 & & 5.0 & 1.0 \\
V835 Cen  & D &  & 1.6 ($\sim 10$) & 2.4 & 2.1 & 1.7 & 3.3 & 2.0 \\
He2--127 & S & & 1.4 ($\sim 10$) & 0.9 & 0.8 & 1.1 & & 0.9 \\
Hen 1092  & S & & 0.6 ($\sim 10$) & 0.6 & 0.4 & 0.9 & & 0.6 \\
HD 330036 & D' & & 0.4 ($\sim 10$) & 0.0 & & & & 0.4 \\
He2--147 & D & 1.0 & & 1.4: & & & 2.0 & 1.0 \\
He2--156 & S & & 1.1 ($\sim 5$) & & & & & 1.1 \\
He2--171 & D & 1.4 &  & 1.8 & 1.1 & 1.5 & 3.3 & 1.4 \\
He2--173 & S & & 0.9 ($\sim 10$) & 0.7 & 0.8 & &  & 0.8 \\
He2--176 & S & 3.6 & 2.3 $\div$ 3.0 & 2.8 & 2.4 & & & 2.8 \\
KX TrA	 & S & & 1.0 ($\sim 10$) & 0.8 & 0.6 & 0.9 & & 0.8 \\
MaC 1--3 & D & 2.2 & & 2.5 & & 2.4 & & 2.3 \\
V455 Sco & S & & 1.0 ($\sim 50$) & 0.8 & 1.1 & 0.7 & 0.9 & 0.9 \\
AS 221	 & S &	& 1.3 ($\sim 5 $) & 1.5 & 1.1 & 1.5 & & 1.3 \\
H2--5	 & D & 1.8 &  & 1.1 & 0.9 & & & 1.0 \\
Th3--7	 & S & 1.6 & 1.0 ($\sim 10$) & & & & & 1.0 \\
Th3--17  & S & 2.3 & 1.1 $\div$ 1.7 & 1.2 & & & & 1.2 \\
Th3--18  & S & 2.1 & 1.3 ($\sim 100$) & 1.2 & 1.0 & & & 1.2 \\
Th3--20  & S & 2.2 & 0.9 $\div$ 1.6 & 1.6 & 2.9: & 0.1: &  & 1.6 \\
Th3--29  & S & 2.7 & 1.4 ($\sim 10$) & 0.8 & & & & 1.4 \\
Th3--30  & S & 2.6 & 1.4 $\div$ 2.0 & 1.1 & 0.8 & & & 1.1 \\
Th3--31  & S & 2.3 & & 1.7 & & & & 1.7 \\
M1--21    & S & 1.0 & & 0.4 & 0.5 & 0.0 & 1.2 & 0.5 \\
He2--251	 & D & 2.9 & & 1.7 & & & & 1.7 \\
W16--296  & S & 2.3 & 1.1 $\div$ 1.8 & 1.2 & & & & 1.2 \\
WR 99	 & S & 2.7 & 2.4 ($\sim 10$) & 2.0 & 2.6 & 2.8 & & 2.4 \\
AE Ara	 & S &	& 0.5 ($\sim 10$) & 0.5 & & & 0.6 & 0.5 \\
UU Ser	  & S & 1.2 & 0 $\div$ 0.6 & 0.7 & 0.4 & 0.2 & & 0.5 \\
AS 241	 & S & 1.4 & & 1.3 & & & & 1.3 \\
He2--275 & S & & 0.8 ($\sim 10$) & 0.9 & & & & 0.9 \\
HD 316285  & S & 1.5 & & 1.6 & &  & & 1.5 \\
V4141 Sgr & D & 1.2 & & 1.3 & & &  1.1 & 1.2 \\
ALS 2	  & S &  & 0.9 ($\sim 10$) & 1.0 & 0.9 & & & 0.9 \\
AS 245	  & S & 2.6 &		   & 2.1 & 1.8 & 1.4 & & 1.8 \\
He2--294 & S & 2.3 & 1.1 $\div$ 1.7  & 0.7 & & & & 1.0 \\
Bl3--6	 & S & 2.1 & & 1.6 & & & & 1.6 \\
MaC 1--9  & S &  & 1.1 ($\sim 5$) & 1.2 & & & & 1.2 \\
V2416 Sgr & S & 2.5 & 1.4 $\div$ 2.0 & 1.2 & 1.4 & 1.2 & 1.7 & 1.4 \\
AS 269	 & ? & 2.4 & & 3.0: & & & & 2.4 \\
Ap1--8 & S &  & 0.8 ($\sim 10$) & 0.6 & & 1.0 & & 0.7 \\
SS 122	  & S & 1.3 &  & 0.9 & 1.6 & 1.1 & & 1.3 \\
H2--38    & D &  & 1.4 ($\sim 10$) & 1.1 & 1.2 & 1.7: & 1.1 & 1.1 \\
SS 129	  & S & 1.6 & 0.4 $\div$ 1.1 & 0.3 &  & &  & 1.0 \\
V615 Sgr & S & 0.5 & & 0.4 & & & & 0.4 \\
AS 280	 & S & 0.0 &	 &	&   &	&      & 0.0 \\
Ap1--9	  & S & 1.3 & & 0.4 & &     & & 0.4 \\
AS 281	  & S &  & 0.9 ($\sim 10$) & 0.7 & 0.8 & 0.0 & 0.5 & 0.7 \\
V2506 Sgr & S & & 0.7 ($\sim 10$) & 0.5 & 0.5 & &  & 0.5 \\
V2756 Sgr & S &  & 0.5 ($\sim 10$ & 0.0 &  & & & 0.5 \\
HD 319167 & S & 1.0 & 0.6 ($\sim 10$) & 0.5 & & & & 0.5 \\
He2--374  & S & & 1.5 ($\sim 5$) & 1.4 &  & &  & 1.4 \\
He2-376   & S & 1.2 & 0 $\div$ 0.6 & 0.2 & & & & 0.6 \\
AS 299	  & S & 1.0 & 0 $\div$ 0.3 & 0.4 & & & & 0.4 \\
V2601 Sgr & S &  & 0.7 ($\sim 10$) &  &  &  & & 0.7 \\
K 3--9	  & D & 2.8 & & 2.0 &  & 2.4 & 2.9 & 2.4 \\
AS 316	  & S & 1.5 & 0.4 $\div$ 1.0 & 0.8 & 0.7 & & & 0.7 \\
AS 323	  & S &  & 0.7 ($ 5 \div 10$) & 0.9 & 0.8 & 0.4 & & 0.9 \\
AS 327	  & S & 1.1 &  & 0.8 & 1.2 & &	1.0 & 1.0 \\
Pe2--16   & S & 2.2 & & 1.6 & & 1.9 & & 1.7 \\
V1413~Aql & S & 0.9 & 0.6 ($5 \div 10$)& 0.0 & & & 0.5 & 0.4 \\
MaC 1--17 & S & 1.2 & & 0.7 & 0.7 & & & 0.7 \\
V352 Aql  & S & & 1.0 ($\sim 10$) & 0.9 & 1.0 & & & 1.0 \\
ALS 1	  & S &  & 0.6 ($5 \div 10$) & 0.6 & 0.4 & & & 0.6 \\
\noalign{\smallskip}
\hline
\end{tabular}
\end{flushleft}
\end{table*}


\begin{table*}
\caption[]{Physical parameters}
\begin{flushleft}
\scriptsize
%\tiny
\begin{tabular}{l c c c l l c r} 
\noalign{\smallskip}
\hline
\noalign{\smallskip}
\multicolumn{1}{l}{Star} & \multicolumn{1}{c}{Type} &
\multicolumn{2}{c}{Sp} & \multicolumn{1}{l}{$d [\mbox{kpc}]$} &
\multicolumn{1}{l}{Ion} &
\multicolumn{1}{c}{$T_{\rm h} [10^3 \mbox{ K}]$} &
\multicolumn{1}{r}{$L_{\rm h} [\mbox{L}_{\odot}]$} \\
     &	 & This study & Other &   &  & & \\
\noalign{\smallskip}
\hline
\noalign{\smallskip}
He2--38    & D & M0 & $\geq$M5 & ~2.2 & O$^{+5}$ & 114 & 13000 \\
He2--87    & S &  & M7 & ~3.5 & O$^{+5}$ & 114 & 700 \\
St2--22     & S & M2 & M & ~5 & He$^{+2}$ & 54 $\div$ 100 & 600 \\
V704 Cen    & D & & & 16 & O$^{+2}$ & 35 $\div$ 55 & 6000 \\
V852~Cen  & D & & M & ~4.3 & He$^{+2}$ & 54 $\div$ 90 & 10000 \\
V835 Cen    & D & & M5 & ~1.9 & O$^{+5}$ & 114 & 28000 \\
He2--127  & S &  & M7+D & 10 & O$^{+5}$ & 114 & 11000 \\
Hen 1092    & S & M5 & K5 & ~5.7 & O$^{+5}$ & 114 & 1700 \\
HD 330036  & D' & & G+D & ~4 & He$^{+2}$ & 54 $\div$ 80 & 1600 \\
He2--147   & D & M7 & M8.5+D & ~3 & He$^{+2}$ & 54 $\div$ 80 & 100 \\
He2--156  & S & K5 & M1 & ~3.4 & O$^{+2}$ & 35 & 3900 \\
He2--171  & D & & M+D & ~5 & O$^{+5}$ & 114 & 12000 \\
He2--173  & S & M3 & M & ~2.8 & He$^{+2}$ & 54 $\div$ 100 & 700 \\
He2--176  & S & & M7 & ~2.6 & O$^{+5}$ & 114 & 4300 \\
KX TrA	   & S & M3 & M6 & ~3 & O$^{+5}$ & 114 & 7500 \\
MaC 1--3   & D & M2 & & (3) & O$^{+5}$ & 114 & $\geq$ 3000 \\
V455 Sco  & S & M1 & M6 & ~2.8 & O$^{+5}$ & 114 & 2000 \\
AS 221	  & S & M1 & M4 & ~4 & O$^{+5}$ & 114 & 1800 \\
H2--5	  & D & M6 & M & ~4.8 & O$^{+5}$ & 114 & 300 \\
Th3--7	  & S & M3 & M5 & ~6 & O$^{+5}$ & 114 & 820 \\
Th3--17   & S & M3 & M3: & ~5 & O$^{+2}$ & 35 $\div$ 55 & 100 \\
Th3--18   & S & M2 & M2: & ~4.2 & O$^{+5}$ & 114 & 750 \\
Th3--20   & S & M3 & M & ~5.2 & O$^{+5}$ & 114 & 2600 \\
Th3--29   & S & M3 & & ~3 & O$^{+5}$ & 114 & 240 \\
Th3--30   & S & M1 & K5 & ~3.8 & O$^{+5}$ & 114 & 100 \\
Th3--31   & S & & M5 & ~4.3 & O$^{+2}$ & 35 $\div$ 55 & 290 \\
M1--21	   & S & M1 & M2 & ~3 & O$^{+5}$ & 114 & 700 \\
He2--251  & D & & & ~8.5 & O$^{+5}$ & 114 & 5700 \\
W16--296   & S & K5 & & (2) & He$^+$ & 24 $\div$ 54 & $\geq$ 100 \\
WR 99	  & S & & & (1) & O$^{+5}$ & 114 & $\geq$ 3000 \\
AE Ara	   & S & M3 & M2 & ~2.3 &  He$^{+2}$ & 54 $\div$ 80 & 1000 \\
UU Ser	   & S & M4 & M & ~6 & O$^{+5}$ & 114 & 1500 \\
AS 241	   & S & M1 & M6 & ~6.3 & He$^+$ & 24 $\div$ 35 & 940 \\
He2--275   & S & M3 & & $\geq$8.5 & O$^{+5}$ & 114 & $\geq$ 960 \\
HD 316285  & S & & & & O$^{+2}$ & 35 $\div$ 55 & \\
V4141~Sgr  & D & & & ~7 & O$^{+2}$ & 35 $\div$ 55 & 1400 \\
ALS 2	   & S & M2 & & (3) & O$^{+5}$ & 114 & 500 \\
AS 245	   & S & M2 & M6 & 4.5 & O$^{+5}$ & 114 & 3500 \\
He2--294   & S & M3 & M3 & ~5.5 & O$^{+5}$ & 114 & 430 \\
Bl3--6	   & S & M3 & & (4) & O$^{+5}$ & 114 & $\geq$ 600 \\
MaC 1--9   & S & M2 & & (3) & He$^{+2}$ & 54 $\div$ 75 & $\geq$ 500 \\
V2416 Sgr  & S & M2 & M5.5 & ~1.3 & O$^{+5}$ & 114 & 460 \\
AS 269	  & ? & & & ~0.6 & He$^+$ & 24 & \\
Ap1--8     & S & M4 & M0 & ~5.3 & O$^{+5}$ & 114 & 570 \\
SS 122	   & S & & M7.5 & ~4.8 & O$^{+5}$ & 114 & 12000 \\
H2--38     & D &  & M8.5 & ~7.2 & O$^{+5}$ & 114 & 20000 \\
SS 129	   & S & K5 & K & ~1.7 & O$^{+5}$ & 115 $\div$ 130 & 100 \\
V615 Sgr   & S & M2 & M & ~3.6 & He$^{+2}$ & 54 $\div$ 65 & 800 \\
AS 280	   & S & & & & He$^{+2}$ & 54 $\div$ 110 & \\
Ap1--9	   & S & K5 & K4 & ~2.5 & He$^{+2}$ & 54 $\div$ 70 & 200 \\
AS 281	   & S & M3 & M5.5 & ~4.5 & O$^{+5}$ & 114 & 2800 \\
V2506 Sgr  & S & M2 & M & ~5 & O$^{+5}$ & 114 & 700 \\
V2756 Sgr  & S & K5 & M2: & ~4 & Ca$^{+4}$ & 67 $\div$ 110 & 900 \\
HD 319167  & S & M3 & M3 & ~4 &  He$^{+2}$ & 54 $\div$ 80 & 1000 \\
He2--374   & S & M4 & M & ~2.5 & Fe$^{+5}$ & 75 $\div$ 100 & 1300 \\
He2-376    & S & M2 & & (4) & O$^{+2}$ & 35 $\div$ 55 & $\geq$ 200 \\
AS 299	   & S & M0 & & ~2.4 & He$^{+2}$ & 54 $\div$ 70 & 430 \\
V2601 Sgr  & S & M5 & M & ~6.1 & He$^{+2}$ & 54 $\div$ 80 & 90 \\
K 3--9	   & D & M3 & & ~3.6 & O$^{+5}$ & 114 & 14000 \\
AS 316	   & S & M3 & M4 & ~4.5 & O$^{+5}$ & 114 & 2000 \\
AS 323	   & S & M3 & & 4.5 & O$^{+5}$ & 114 & 1200 \\
AS 327	   & S & M0 & M2 & ~3 & O$^{+5}$ & 114 & 2700 \\
Pe2--16    & S & K5 & M5 & ~5.5 & O$^{+5}$ & 114 & 6200 \\
V1413~Aql  & S & M0 & M5 & ~5 & O$^{+2}$ & 35 $\div$ 55 & 400 \\
MaC 1--17  & S & M1 & & (7) & He$^{+2}$ & 54 $\div$ 90 & $\geq$ 740 \\
V352 Aql   & S & M3 & & $\geq$9.6 & O$^{+5}$ & 114 & $\geq$ 1600 \\
ALS 1	   & S & M3 & & (6) & He$^{+2}$ & 54 $\div$ 80 & $\geq$ 500 \\
\noalign{\smallskip}
\hline
\end{tabular}
\end{flushleft}
\end{table*}


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