\begin{table}%t3
\caption{Adopted stellar parameters and results.}\label{table:3}
%\centerline
{\begin{tabular}{l l l r l r r r r r r } 
\hline\hline\noalign{\smallskip}
Star & Sp. type & $T_{\rm eff}$ & $\log(L_*/{L}_\odot)$& $\log(g)$ & $M_*$ &  $\eta$ & $\dot{M}$ & $e_{\dot{M}}$  & $\dot{M}_{\rm pred}$ & $\dot{M}_{\rm H\alpha}$ \\
     &          &   (K)         &                          &          &  ($M_\odot$)   &&
      \multicolumn{4}{c}{(~$10^{-6}~~~~$$M_\odot~~~~$ yr$^{-1}~$)} \\
\hline
HD~156154 & O8 Iab(f)&  33179$^a$ &  5.68$^a$& 3.10& 19.2 &            & $<$4.4&      &    3.2&       \\
HD~151804 &  O8 Iaf  &  29000$^b$ &  5.88$^b$& 3.00& 41.4 &$1.0\pm0.12$&    10.4&  3.70&    3.2&  16.0$^b$ \\
BD-11 4586&  O8 Ib(f)&  33179$^a$ &  5.68$^a$& 3.10& 19.2 &            & $<$5.6&      &    3.2&   (2.6)$^c$ \\
HD~112244 &O8.5 Iab(f)& 32274$^a$ &  5.65$^a$& 3.10& 20.0 &            & $<$3.0&      &    2.6&       \\
HD~76341  &  O9 Ib   &  31368$^a$ &  5.61$^a$& 3.05& 18.2 &$1.3\pm0.17$&     7.2&  2.51&    2.1&       \\
CygOB2-10 &  O9.5 I  &  29700$^d$ &  5.82$^d$& 3.00& 32.8 &$0.5\pm0.07$&     4.4&  1.77&    2.7&   2.7$^{d,e}$ \\
HD~195592 &  O9.5 I  &  29000$^f$ &  5.60$^f$& 3.00& 21.7 &$1.0\pm0.14$&     4.8&  1.69&    1.2&   3.8$^d$ \\
HD~30614  &  O9.5 Ia &  29000$^f$ &  5.63$^f$& 3.00& 23.3 &$0.6\pm0.08$&     3.3&  1.22&    1.5&   5.0$^f$ \\
HD~209975 &  O9.5 Ib &  32000$^d$ &  5.31$^d$& 3.10&  9.5 &$1.2\pm0.15$&     2.4&  0.94&    0.7&   1.1$^d$ \\
HD~37742  &  O9.7 Ib &  28500$^f$ &  5.57$^a$& 2.95& 19.4 &$0.4\pm0.05$&     1.5&  0.49&    0.9&   (1.8)$^g$ \\
HD~47432  &  O9.7 Ib &  28500$^f$ &  5.57$^a$& 2.96& 19.8 &            & $<$3.1&      &    1.1&   (1.9)$^h$ \\
HD~152424 &  OC9.7 Ia&  28500$^f$ &  5.57$^a$& 2.96& 19.8 &$1.0\pm0.14$&     4.5&  1.65&    1.0&       \\
HD~37128  &  B0 Ia   &  27000$^f$ &  5.44$^f$& 2.90& 15.9 &$0.5\pm0.07$&     1.6&  0.54&    0.5&   2.3$^f$ \\
HD~204172 &  B0 Ib   &  27500$^f$ &  5.50$^f$& 2.93& 18.2 &            & $<$5.0&      &    0.7&       \\
HD~163181 &  BN0.5 Iap& 26000$^f$ &  5.57$^a$& 2.85& 22.4 &$0.1\pm0.02$&     2.1&  0.73&    2.5&       \\
HD~154090 &  B0.7 Ia &  22500$^f$ &  5.48$^f$& 2.60& 18.1 &$0.2\pm0.03$&     1.3&  0.48&    3.2&   1.0$^f$ \\
HD~2905   &  BC0.7 Ia&  21500$^f$ &  5.52$^f$& 2.53& 20.3 &$0.4\pm0.05$&     2.5&  0.84&    2.3&   2.0$^f$ \\
HD~169454 &  B1 Ia   &  21500$^f$ &  5.45$^f$& 2.53& 17.3 &$0.5\pm0.06$&     3.4&  1.14&    2.9&       \\
HD~157246 &  B1 Ib   &  20800$^i$ &  5.45$^f$& 2.45& 16.4 &            & $<$0.6&      &    3.4&       \\
BD-14 5037&  B1.5 Ia &  20500$^f$ &  5.60$^f$& 2.45& 24.5 &$0.2\pm0.04$&     2.5&  1.18&    4.9&   (3.4)$^j$ \\
HD~152236 &  B1.5 Ia+&  18000$^f$ &  6.10$^f$& 2.20& 73.4 &$0.1\pm0.02$&     8.3&  2.70&   41.7&     6$^f$ \\
HD~190603 &  B1.5 Ia+&  18500$^f$ &  5.57$^f$& 2.25& 21.8 &            & $<$2.1&      &    6.8&   2.5$^f$ \\
HD~148379 &  B1.5 Iape& 18500$^b$ &  5.56$^b$& 2.25& 21.3 &$0.1\pm0.01$&     0.8&  0.29&    5.8&   1.5$^b$ \\
HD~194279 &  B2 Ia   &  19000$^f$ &  5.37$^f$& 2.30& 13.9 &$0.2\pm0.02$&     1.5&  0.58&    3.3&   1.1$^f$ \\
HD~41117  &  B2 Ia   &  19000$^f$ &  5.65$^f$& 2.30& 26.4 &$0.1\pm0.02$&     2.1&  0.76&    8.5&   1.0$^f$ \\
HD~80077  &  B2 Ia+  &  18500$^f$ &  5.40$^f$& 2.25& 14.7 &$0.1\pm0.01$&     1.7&  0.69&   30.2&       \\
HD~165024 &  B2 Ib   &  18000$^f$ &  5.40$^f$& 2.20& 14.7 &            & $<$0.6&      &    0.9&       \\
HD~198478 &  B2.5 Ia &  16500$^f$ &  5.03$^f$& 2.05&  6.3 &            & $<$0.5&      &    1.1&   0.2$^f$ \\
HD~42087  & B2.5 Ib  &  19000$^b$ &  5.08$^b$& 2.30&  7.1 &            & $<$1.1&      &    0.9&   0.2$^b$ \\
HD~43384  & B3 Iab   &  15500$^f$ &  4.88$^h$& 1.95&  4.4 &            & $<$1.7&      &    0.3&   (0.3)$^h$ \\
 \hline
\end{tabular}}
\smallskip
$^a$Martins et~al. (\cite{martins05}); $^b$this work; $^c$Scuderi et~al. (\cite{scuderi92}); $^d$Puls et~al. (\cite{puls06}); $^e$Herrero et~al. (\cite{herrero02}); $^f$Crowther et~al. (\cite{crowt06}); $^g$Lamers \& Leitherer (\cite{lamer93}); $^h$Morel et~al. (\cite{morel04}); $^i$Lamers et~al. (\cite{lamer95}); $^j$Scuderi et~al. (\cite{scuderi98}). 
\end{table}