\begin{table}%t2
\caption{Stellar parameters for the four groups of peculiar O-type
stars.} \label{t_params}
%\centerline
{
\begin{tabular}{lccccccccc}
\hline
Name & $\log (L/\lsun)$ & $\teff$ & $\log g$ & $M$       & $R$       & $\vinf$ & log$\mdot$ & $\rho_{\rm wind}$ & $v \sin i$ \\
     &                & (kK)    &        & $(\msun)$ & $(\rsun)$ & (km/s)  & ($\msunyr$) & ($10^{-13}$ \msunyr/\kms${\rsun^2}$) & (km/s)\\
\hline
\\
\multicolumn{10}{l}{Group I~~{\it OVz and weak wind dwarfs}}\\
$\Theta^1$ Ori C    &  5.13  & 39  & 4.1  & 30   & 8  & 580 & $-5.7$ & 530 & 24\\
$\Theta^2$ Ori A    & 4.62  & 30.5 & 3.92 & 17 & 7  & 2500$^1$    & $-7.59$ & 1.9      \\
HD 42088 & 5.23  & 38   &   4.0 & 32        & 10 & 1900 & $-6.19$ & 37 & 60 \\
HD 54662           & 5.2   & 36.8 & 3.92 & 29 & 10  & 2456& $-6.40$ & 17 &  73   \\
HD 152590          & 5.00  & 34.4 & 3.92 & 24 & 9  & 1785& $-6.64$ & 23 & 60    \\
HD 93128           &  5.66 & 46.5 & 4.00 & 40 & 10 & 3210$^1$    & $-5.53$ & 100 & 100 \\
HD 93129B          &  5.86 & 44.0 & 3.92 & 52 & 13 & 3210$^1$    & $-5.25$ & 110 &      \\
CPD$-58$\degree 2611 &  5.3  & 38.2 & 3.92 & 32 & 10 & 2870$^1$    & $-6.23$ & 21  &      \\
CPD$-58$\degree 2620 &  5.2  & 36.8 & 3.92 & 29 & 24 & 1760$^1$    & $-6.43$ & 15 & 110     \\
\\
\multicolumn{10}{l}{Group II~~{\it Of?p}}\\
HD 148937     &     5.75  & 41.0  & 4.0  & $\sim$55   & 15 & 2285 & $-5.45$ & 71 & 76 \\
HD 108        &     5.40  & 37.0  & 3.75 & $\sim$35   & 12 & 1960 & $-5.97$ & 37 & 78 \\
HD 191612     &     5.4   & 35    & 3.5  & $\sim$35   & 15 & 2450$^1$  & $-6.14$ & 17    \\
\\
\multicolumn{10}{l}{Group III~~{\it Oe stars}}\\
HD 39680  & 5.5  & 40   &       & 45        & 11   & 1675 & $-5.69$ & 90 & 218   \\
HD 45314 & 4.72  & 31.5 & 3.92  & 18        & 8  & 2410$^1$     & $-7.37$ & 3.0  & 285 \\
HD 46485  & 5.1  & 35.5 & 3.92  & 27      & 9  & 1800 & $-6.44$ & 25 &       \\
HD 60848  & 4.9  & 33.4 & 3.92  & 22        & 8.5  & 1765 & $-6.84$ & 12 & 240   \\
HD 120678 & 4.9  & 33.4 & 3.92  & 22        & 8.5  & 2580$^1$ & $-7.02$ & 5.5 &     \\
Zeta Oph & 4.88  & 32.1 & 3.62  & 20        & 9  & 1505 & $-6.83$ & 12 & 372   \\
HD 155806 & 4.9  & 33.4 & 3.92  & 22        & 8.5  & 2460 & $-7.02$ & 5.5 & 91   \\
\\
\multicolumn{10}{l}{Group IV~~{\it Onfp}}\\
HD 152248A & 5.69 & 33.3 & 3.4  & 41   & 21.1 & 2420 & $-6.10$ & 16 & 159    \\
HD 210839 & 5.83 & 36.0 & 3.55  & 62   & 21.1 & 2250 & $-5.47$ & 33 & 200 \\
Zeta Pup  & 5.90 & 39.0 & 3.60  & 54   & 19.4 & 2250 & $-5.24$ & 68 & 219  \\
Cyg OB2 No. 5 & 5.69 & 33.3 & 3.4& 41   & 21.1 & 2240$^1$ & $-5.64$ & 27      \\
\hline
\end{tabular}}
The stellar parameters are taken from the following papers:
Repolust et~al. (\cite{Repolust2004}), Martins et~al.
(\cite{Martins2005b}), and Puls et~al. (\cite{Puls2006}). For all
stars without recent line-blanketed models, the calibrations of
Martins et~al. (\cite{Martins2005a}) are used. The mass-loss rates
are from Monte Carlo radiation-driven wind models (Vink et~al.
\cite{Vink2000}). The wind density is given as $\rho_{\rm
wind}=\mdot/(R^2 \vinf)$.
Where spectral subtypes are not provided, we interpolate. $v\sin i$ are mostly taken from Howarth et~al. (\cite{Howarth1997}).\\
$^1$ Note that the terminal velocity is calculated by
multiplication of the escape velocity
by the canonical factor of 2.6 (Lamers et~al. \cite{Lamers1995}).
\end{table}