\begin{table}%t3
\caption
{Final results for our sample of Galactic B-SGs: Stellar and wind
parameters adopted ($\rightarrow$\MV) and derived using FASTWIND. \Teff in kK, 
\Rstar in \Rsun, \Mstar in \Msun, \vinf in \kms, \Mdot in $10^{-6}$~{$M_{\odot}$/yr}.  
$D_{\rm mom}$ (in cgs-units) denotes the modified wind-momentum rate.
High precision $\beta$-values are given bold-faced. For non-tabulated errors, see text.}
\label{para_2}
%\begin{center}
\par
\begin{tabular}{llccccclcrrlll}
\hline 
\hline
\multicolumn{1}{c}{Object}
&\multicolumn{1}{l}{Sp}
&\multicolumn{1}{r}{\MV}
&\multicolumn{1}{c}{\Teff}
&\multicolumn{1}{c}{\logg}
&\multicolumn{1}{c}{\loggtr}
&\multicolumn{1}{c}{\Rstar}
&\multicolumn{1}{c}{\Yhe}
&\multicolumn{1}{c}{\logl}
&\multicolumn{1}{r}{\Mstar}
&\multicolumn{1}{r}{\vinf}
&\multicolumn{1}{c}{$\beta$}
&\multicolumn{1}{c}{log \Mdot}
&\multicolumn{1}{l}{\logwm}
\\
\hline
HD 185859  &B0.5 Ia  &--7.00 &26.3 &2.95 &2.96 &35  &$0.10\pm0.02$ &5.72  &$41^{\rm +27}_{\rm -16}$ &1~830 &${\bf1.1}\pm0.1^{a}$ &$-5.82\pm0.13$     &$29.01\pm0.20$ \\ 
HD 190603  &B1.5 Ia+ &--8.21 &19.5 &2.35 &2.36 &80  &$0.20\pm 0.02$ &5.92  &$53^{\rm +41}_{\rm -23}$ &485    &${\bf2.9}\pm0.2$        &--$5.70\pm0.16$     &$28.73\pm0.22$ \\  
             &         &--7.53& &     &2.36 &58&    &5.65&$28^{\rm +21}_{\rm -12}$ &      &                    &--$5.91\pm0.16$    &$28.45\pm0.22$ \\  
HD 206165  &B2 Ib    &--6.19 &19.3 &2.50 &2.51 &32  &0.10--0.20   &5.11  &$12^{\rm +7}_{\rm -4}$ &640&${\bf1.5}^{\rm +0.2}_{\rm -0.1}$ $^{a)}$&--$6.57\pm0.13$ &$27.79\pm0.17$ \\  
HD 198478  &B2.5 Ia  &--6.93 &17.5 &2.10 &2.12 &49  &0.10--0.20   &5.31  &$11^{\rm +5}_{\rm -3}$  &200...470&${\bf1.3}\pm0.1$      &--6.93...--6.39       &26.97...27.48 \\ 
             &         &--6.37& &     &2.12 &38  &              &5.08&$7^{\rm +3}_{\rm -2}$   &       &                &--7.00...--6.46  &26.84...27.36 \\ 
HD 191243  &B5 Ib    &--5.80 &14.8 &2.60 &2.61 &34  &$0.09\pm0.02$ &4.70 &$17^{\rm +9}_{\rm -6}$ &470 &0.8...1.5  &$-7.52^{\rm+0.26}_{\rm-0.20}$     &$26.71^{\rm+0.27}_{\rm-0.23}$ \\ 
             &  &--6.41 &     &     &2.60 &46  & &4.96  &$31^{\rm +17}_{\rm -11}$ & &   &$-7.30^{\rm+0.25}_{\rm-0.17}$       &$27.00^{\rm+0.25}_{\rm-0.21}$\\  
HD 199478  &B8 Iae   &--7.00 &13.0 &1.70 &1.73 &68  &$0.10\pm0.02$ &5.08  &$9^{\rm +5}_{\rm -3}$   &230    &0.8...1.5       &--6.73...--6.18               &27.33...27.88 \\ 
HD 212593  &B9 Iab   &--6.50 &11.8 &2.18 &2.19 &59  &0.06--0.10   &4.79  &$19^{\rm +13}_{\rm -8}$  &350    &0.8...1.5       &$-7.04^{\rm+0.25}_{\rm-0.19}$      &$27.18^{\rm+0.28}_{\rm-0.24}$\\
HD 202850  &B9 Iab   &--6.18 &11.0 &1.85 &1.87 &54  &$0.09\pm0.02$ &4.59  &$8^{\rm +4}_{\rm -3}$   &240    &0.8...1.8       &$-7.22^{\rm+0.25}_{\rm-0.17}$      &$26.82^{\rm+0.25}_{\rm-0.20}$\\
\hline
\end{tabular}
%\end{center}
\par
$^{a}$ \Ha (though in absorption) indicates $\beta > 1$.  
\end{table}