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\begin{table*}
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\caption{Atmospheric parameters and evolutionary state for He-r stars
obtained using Kurucz models. The quantities with the ``{\it new}''
superscript have been obtained assuming corrected the photometric T$_{eff}$
, while the others have been obtained only from the Balmer line
profiles.}
\begin{tabular}{|r|r|r|r|r|r|r|r|r|r|}\hline   
 Star & T$_{eff}$& log g& T$^{new}_{eff}$& log g$^{new}$& $R/R_{z}$
& He abundance & $R/R_{z}^{new}$ & He$^{new}$& emis.\\ \hline
36485 & 18000 & 4.4 $\pm$ 0.11 & 18400& 4.5 $\pm$ 0.27 & 0.85 $\pm$ 0.11&
0.14 $\pm$ 0.07 & 0.76 $\pm$0.24 & 0.15& \\ 
37017 & 18500 & 4.3 $\pm$ 0.10& 19200& 4.4 $\pm$ 0.16 & 0.95 $\pm$ 0.11&
0.14 $\pm$ 0.08 & 0.85 $\pm$0.16 & 0.12&  \\
37479 & 22000 & 4.5 $\pm$ 0.17& 22200& 4.3 $\pm$ 0.29 & 0.76 $\pm$ 0.15&
0.22 $\pm$ 0.09 & 1.01 $\pm$0.34& 0.32& e \\
37776 & 22000 & 4.5 $\pm$ 0.07& 21800& 4.3 $\pm$ 0.32& 0.76 $\pm$ 0.06& 0.19
$\pm$ 0.09 & 0.95 $\pm$0.35 & 0.22&  \\
260858& 18000 & 4.0 $\pm$ 0.10& 19200& 4.3 $\pm$ 0.15& 1.35 $\pm$ 0.16& 0.24
$\pm$ 0.10 & 0.95 $\pm$0.16 & 0.19& \\
264111& 22400 & 4.2 $\pm$ 0.06& 23200& 4.3 $\pm$ 0.35& 0.85 $\pm$ 0.06& 0.20
$\pm$ 0.11 & 0.95 $\pm$0.38 & 0.30& \\
$-27^\circ 3748$ & 23000& 4.5 $\pm$ 0.11& 22700&4.3 $\pm$ 0.30&  0.76
$\pm$ 0.10 & 0.13 $\pm$ 0.06 & 0.95 $\pm$0.33 & 0.18&  \\
58260 & 19000 & 4.0 $\pm$ 0.19 & 19000& 4.25$\pm$ 0.16& 1.35 $\pm$ 0.29& 0.27
$\pm$ 0.10 & 1.01 $\pm$0.19 & 0.21& e \\
60344 & 21000 & 4.5 $\pm$ 0.18 & 21700& 4.2 $\pm$ 0.27 & 0.76 $\pm$ 0.16&
0.16 $\pm$ 0.10 & 1.06 $\pm$0.32 & 0.21& \\
64740 & 21000 & 4.5 $\pm$ 0.06& 22700& 4.3 $\pm$ 0.30& 0.76 $\pm$ 0.05& 0.13
$\pm$ 0.08 & 0.99 $\pm$0.34 & 0.18& \\
66522 & 18000 & 4.0 $\pm$ 0.10& 18800& 4.3 $\pm$ 0.16& 1.35 $\pm$ 0.16& 0.38
$\pm$ 0.12 & 0.99 $\pm$0.18 & 0.32& \\
68450 & 32500 & 4.0 & 32300& 4.05& ---& --- & ---& ---& e \\
$-46^\circ 4639$ & 22500& 4.5 $\pm$ 0.11& 22000&4.3 $\pm$ 0.40&  0.76
$\pm$ 0.11  & 0.13 $\pm$ 0.08 & 0.95 $\pm$0.44 & 0.22& \\
92938 & 15000 & 4.0 $\pm$ 0.10& 15000& 4.1 $\pm$ 0.14& 1.35 $\pm$ 0.16& 0.20
$\pm$ 0.08 & 1.20 $\pm$0.19& 0.20&  \\
96446 & 20500 & 4.4 $\pm$ 0.21& 22000& 4.5 $\pm$ 0.70 & 0.85 $\pm$ 0.21&
0.38 $\pm$ 0.12 & 0.76$\pm$0.60 & 0.37&e \\
$-62^\circ 2124$ & 26000& 4.2 $\pm$ 0.21& ---&---&  1.07
$\pm$ 0.26 & $\sim$ 0.81 $\pm$ 0.15 & --- & ---& e(H) \\
108483& 19200 & 4.3 $\pm$ 0.10& 19100& 4.2 $\pm$ 0.16& 0.76 $\pm$ 0.09& 0.12
$\pm$ 0.05 & 1.07 $\pm$0.20 & 0.11& \\
124448& ---& --- & 22000  & 3.7 $\pm$0.21& 1.91 $\pm$ 0.46 &  $<$0.8
?      & --- & $<$0.8& e(H) \\
133518& 17500 & 4.0 $\pm$ 0.10& 18600& 4.3 $\pm$ 0.15 & 1.35 $\pm$ 0.16 &
0.29 $\pm$ 0.10 & 0.95 $\pm$0.16 & 0.23& \\ \hline
56139  & --- & ---& 18000 & 3.6 $\pm$0.18&  --- & --- 
& 2.14 $\pm$0.44 & 0.12 $\pm$0.05 & e(H) \\
105435 & ---& ---& 26000& 4.2 $\pm$0.21 & --- & ---
& 1.07 $\pm$0.26 & 0.08 $\pm$ 0.05 & e(H) \\
110879 & 18000 & 4.4 $\pm$ 0.07& 18200& 4.2 $\pm$ 0.15& 0.76 $\pm$ 0.06&
0.10 $\pm$ 0.05 & 1.07 $\pm$0.18 & 0.11& \\
121790 & 19500 & 4.4 $\pm$ 0.11& 19600& 4.1 $\pm$ 0.16& 0.76 $\pm$ 0.10&
0.10 $\pm$ 0.06 & 1.15 $\pm$0.21 & 0.12& \\  
122980 & 18500 & 4.4 $\pm$ 0.10& 19600& 4.2 $\pm$ 0.16& 0.76 $\pm$ 0.09&
0.11 $\pm$ 0.06 & 1.10$\pm$0.20& 0.12& \\ \hline
\end{tabular}
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\end{table*}
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