\begin{table}%t10
%\centering
\par
\caption{\label{tab:bkpeg_absdim}Astrophysical data for BK~Peg.}
%%\centerline
\begin{tabular}{lrr} \hline    
\hline    
\noalign{\smallskip}    
                     &    Primary       &    Secondary      \\ 
\noalign{\smallskip}    
\hline    
\noalign{\smallskip}    
Absolute dimensions:          &                   &                 
 \\ 
$M/M_{\odot}$                  &$1.414 \pm 0.007$  &$1.257 \pm 0.005$
\\ 
$R/R_{\odot}$                  &$1.988 \pm 0.008$  &$1.474 \pm 0.017$ 
\\ 
$\log g$ (cgs)                & $3.992 \pm 0.004$ & $4.201 \pm 0.010$
\\
%$v \sin i$ (\kms)             & $14.1\pm0.1$        & $12.1\pm0.2$   %from w1,2 in srf/vrot.jvc
$v \sin i$\tablefootmark{a} (\kms)  & $16.6 \pm 0.2$    & $13.4 \pm 0.2$ \\  %rsrf080930
$v_{\rm sync}$\tablefootmark{b} (\kms)  & $18.3 \pm 0.1$    & $13.6 \pm 0.2$ \\ 
$v_{\rm psync}$\tablefootmark{c} (\kms) & $18.3 \pm 0.1$    & $13.6 \pm 0.2$ \\ 
$v_{\rm peri}$\tablefootmark{d} (\kms)  & $18.5 \pm 0.1$    & $13.7 \pm 0.2$ \\ 
 & & \\ 
Photometric data:             &                   &                 
\\ 
$V$\tablefootmark{e}     &     $10.473 \pm 0.009$  &        $11.080 \pm 0.014$\\  %jvc080828 
$(b-y)$\tablefootmark{e} &     $ 0.363 \pm 0.007$  &        $ 0.360 \pm 0.008$\\
$m_1$\tablefootmark{e}    &     $ 0.144 \pm 0.013$  &        $ 0.139 \pm 0.016$\\
$c_1$\tablefootmark{e}  &     $ 0.466 \pm 0.014$  &        $ 0.436 \pm 0.017$\\
$E(b-y)$    & \multicolumn{2}{c}   {$0.044 \pm 0.015$} \\
%          &              &               \\
$T_{\mbox{\scriptsize eff}}~$      &  $6265 \pm  85$    &   $6320 \pm  90$ \\
$M_{\mbox{\scriptsize bol}}~$      &  $2.90  \pm 0.06$  &   $3.51  \pm 0.07$ \\
$\log L/L_{\odot}$ & $0.74 \pm 0.02$ &    $0.49 \pm 0.03$ \\
$B.C.$            & $-0.01$         &    $-0.01$ \\
$M_V$ &             $ 2.91 \pm 0.06$&   $ 3.52 \pm 0.07$ \\
%                 &                 &             \\
%$V-M_V$          &$ 7.57  \pm 0.06 $& $ 7.57  \pm 0.07 $ \\
$V_0-M_V$         &$ 7.37  \pm 0.09 $& $  7.37  \pm 0.10 $ \\
Distance ~ (pc) &$ 298   \pm  12  $& $ 298   \pm  13  $ \\
 & & \\ 
Abundance:                    &                   &   \\              
\feh\       & \multicolumn{2}{c}   {$-0.12 \pm 0.07$} \\        
\hline
\end{tabular}            %}
\tablefoot{\tablefoottext{a}{Observed rotational velocity.}
\tablefoottext{b}{Equatorial velocity for synchronous rotation.}
\tablefoottext{c}{Equatorial velocity for pseudo-synchronous rotation.}
\tablefoottext{d}{Refers to periastron velocity.}
\tablefoottext{e}{Not corrected for interstellar absorption/reddening.}
Bolometric corrections ($BC$) by Flower (\cite{flower96}) have been
assumed, together with
$T_{\rm eff\odot} = 5780$ K, $BC_{\odot} = -0.08$, and $M_{bol\odot} = 4.74$.}
\end{table}