\begin{table}%t2
%\centering
\par
%\renewcommand{\arraystretch}{1.03}
  \caption{Effective temperature and surface gravity determinations.\label{tab2}}
  \begin{tabular}{crrl}
\hline\hline
Star & $T_{\rm eff}$ (K) &       ${\rm Log}~ g$ & Method \\
\hline
$\theta$ And & 8968 & 3.87 & Napiwotzki et~al. (\cite{Napiwotzki93}) with {$uvby\beta$}
photometry\\
  & 9000 & 4.00 & Spectrophotometry and H$\gamma$ profile fitting, solar model\\
       &      &      &  \\
$\epsilon$ Del& 13755 & 3.65 & Napiwotzki et~al. (\cite{Napiwotzki93}) with {$uvby\beta$}
  photometry\\
              & 13679 & 3.65 & same with correction from Adelman et~al. (\cite{Adelman02})\\
              & 13679 & 3.65 & same with H$\beta$ fitting \\
       &      &      &  \\
$\epsilon$ Aqr & 9229 & 3.56 & Napiwotzki et~al. (\cite{Napiwotzki93}) with {$uvby\beta$}
photometry\\
  & 9200 & 3.50 & Spectrophotometry and H$\gamma$ profile fitting, solar model\\
  & 9050 & 3.75 & Spectrophotometry and H$\gamma$ profile fitting, solar model,
 iron equilibrium\\
       &      &      &  \\
$\iota$ And   & 11845 & 3.35 & Napiwotzki et~al. (\cite{Napiwotzki93}) with {$uvby\beta$}
photometry\\
              & 11600 & 3.35 & Spectrophotometry and H$\beta$ profile fitting,
solar model\\
\hline
\end{tabular}
\end{table}