\begin{table}%t2 %\begin{center} \par \caption{\label{Table:Results}Effective temperatures, gravities and metallicities.} \small \begin{tabular}{lrc} \hline\hline Star & $T_{\rm eff}$~(K)& $\log g_*$ \\ \hline HD 58647 & 10~500$^1$ & $3.33\pm0.05$ \\ HD 150193 & 8970$^1$ & $3.99\pm0.12$ \\ HD 179218 & 9500$^1$ & $3.91\pm0.07$ \\ HD 190073 & 9500$^1$ & $3.37\pm0.08$ \\ HR 26 A & 11~400$^2$ & $4.08\pm0.05$ \\ AS 442 & 11~000$^7$ & $3.79\pm0.10$ \\ BD+31 643 & 15~400$^1$ & $3.75\pm0.05$ \\ V346 Ori & 9750$^7$ & $3.96\pm0.11$ \\ V350 Ori & 8970$^7$ & $4.07\pm0.12$ \\ \end{tabular} %\centerline {\begin{tabular}{lrcr} \hline Star & $T_{\rm eff}$~(K) & $\log g_*$ & \multicolumn{1}{c}{[M/H]} \\ \hline HD 31648 & 8250$^7$ &$4.00\pm0.20$ &$0.00\pm0.05$ \\ HD 163296 & 9250$^7$ &$4.07\pm0.09$ &$+0.20\pm0.10$ \\ HR 10 & 9750$^7$ &$3.72\pm0.10$ &$+0.20$: \\ HR 2174 & 8970$^1$ &$3.08\pm0.12$ &$0.00\pm0.10$ \\ HR 4757 A & 10~400$^{2,7}$ &$4.06\pm0.05$ &$+0.10\pm0.10$ \\ HR 5422 A & 10~250$^7$ &$4.08\pm0.06$ &$+0.20\pm0.10$ \\ HR 9043 & 7570$^3$ &$3.85\pm0.10$ &$0.00\pm0.10$ \\ $\lambda$ Boo & 8750$^4$ &$4.10\pm0.12$ &$-1.50\pm0.20$ \\ VX Cas & 10~000$^7$ &$4.27\pm0.05$ &$0.00\pm0.10$ \\ SV Cep & 10~250$^{5,7}$ &$4.25\pm0.10$ &$+0.10\pm0.10$ \\ 49 Cet & 9500$^7$ &$4.30\pm0.11$ &$+0.10\pm0.10$ \\ 24 CVn & 9000$^7$ &$3.81\pm0.13$ &$+0.80\pm0.10$ \\ 51 Oph & 10~250$^7$ &$3.57\pm0.06$ &$+0.10\pm0.10$ \\ T Ori & 9750$^7$ &$4.03\pm0.10$ &$+0.10\pm0.10$ \\ BF Ori & 8970$^1$ &$3.83\pm0.12$ &$+0.20\pm0.05$ \\ UX Ori & 8460$^1$ &$3.89\pm0.15$ &$0.00\pm0.10$ \\ XY Per & 9750$^7$ &$3.86\pm0.16$ &$+0.80$: \\ VV Ser & 13~800$^{6,7}$ &$4.02\pm0.15$ &$0.00$: \\ 17 Sex & 9520$^1$ &$3.19\pm0.10$ &$+0.10\pm0.10$ \\ RR Tau & 10~000$^7$ &$3.31\pm0.13$ &$+0.10\pm0.05$ \\ WW Vul & 8970$^1$ &$3.90\pm0.20$ &$+0.50\pm0.10$ \\ \hline \end{tabular}} \parbox{8.8cm}{ Notes to Table~\ref{Table:Results}: the effective temperatures are from $^1$~Mer\'{\i}n (\cite{Merin2004a}); $^2$~Gerbaldi et~al. (\cite{Gerbaldi2001}); $^3$~Paunzen et~al. (\cite{Paunzen2006}); $^4$~adopted as a mean of the values proposed by Venn \& Lambert (\cite{Venn1990}) and Adelman et~al. (\cite{Adelman2002}); $^5$~Mora et~al. (\cite{Mora2004}); $^6$~Hern\'andez et~al. (\cite{Hernandez2004}); $^7$~this work.} %\end{center} \end{table}