\begin{table}%t1
   \caption{\label{t:mag}Visual and absolute magnitudes, $B-V$ color, Hipparcos 
              parallaxes, stellar masses (derived iterativey during the
              abundance analysis using the spectroscopic
              temperatures and abundances), and projected binary separation 
              for program stars. The formal errors
              on magnitudes and colors are probably underestimated (see Paper~I).}
     \small%\centering
\par
            \begin{tabular}{lccccccccccc}
         \hline\hline
                 Object      &  $V_{\rm A}$ &  $V_{\rm B}$   & 
		 $(B-V)_{\rm A}$ & $(B-V)_{\rm B}$  & $\pi$  & $M_{V({\rm A})}$
		   & $M_{V({\rm B})}$ & $M_{\rm A}$ & $M_{\rm B}$ & $\rho$ & $\rho$ \\
         &  &  & &  & mas  &  &  & $M_{\odot}$ & $M_{\odot}$ & $''$ & AU \\
         \hline
  \object{HIP~3290} &$7.995\pm0.004$&$8.986\pm0.011$&$0.473\pm0.015$&$0.514\pm0.028$&$ 10.33\pm1.22$&$ 2.95\pm0.26$&$3.94\pm0.26$& 1.05 & 0.96 &  6.3 & 645 \\
\object{HIP~10175} &$8.180\pm0.006$&$8.647\pm0.010$&$0.674\pm0.026$&$0.732\pm0.046$&$ 20.41\pm1.75$&$ 4.67\pm0.19$&$5.14\pm0.19$& 1.00 & 0.92 &  5.9 & 298 \\
\object{HIP~20552} &$6.839\pm0.004$&$7.238\pm0.005$&$0.630\pm0.014$&$0.704\pm0.015$&$ 36.92\pm0.84$&$ 4.67\pm0.05$&$5.07\pm0.05$& 1.08 & 1.01 &  5.6 & 152 \\
\object{HIP~37918/23} &$8.167\pm0.012$&$8.266\pm0.011$&$0.779\pm0.029$&$0.785\pm0.023$&$ 29.20\pm1.91$&$ 5.46\pm0.14$&$5.56\pm0.14$& 0.98 & 0.95 & 23.1 & 802 \\ 
\object{HIP~39409} &$9.253\pm0.009$&$9.312\pm0.009$&$0.747\pm0.053$&$0.669\pm0.051$&$ 15.11\pm2.71$&$ 4.85\pm0.39$&$4.91\pm0.39$& 0.99 & 0.98 &  5.1 & 390 \\
\object{HIP~44814/17} &$9.495\pm0.004$&$9.826\pm0.005$&$0.843\pm0.049$&$0.859\pm0.060$&$ 15.80\pm2.89$&$ 5.18\pm0.40$&$5.51\pm0.40$& 0.97 & 0.92 & 10.6 & 774 \\
\object{HIP~49520} &$8.686\pm0.009$&$8.849\pm0.011$&$0.617\pm0.033$&$0.599\pm0.038$&$ 19.63\pm2.11$&$ 5.06\pm0.23$&$5.22\pm0.23$& 1.00 & 0.99 &  9.6 & 508 \\
\object{HIP~51266} &$8.369\pm0.006$&$8.606\pm0.007$&$0.830\pm0.024$&$0.818\pm0.030$&$ 29.86\pm1.64$&$ 5.72\pm0.12$&$5.96\pm0.12$& 0.93 & 0.89 &  5.9 & 199 \\
\object{HIP~55288} &$7.051\pm0.006$&$7.814\pm0.010$&$0.504\pm0.013$&$0.710\pm0.023$&$ 17.98\pm1.60$&$ 3.26\pm0.19$&$4.02\pm0.19$& 1.21 & 1.03 &  9.5 & 542 \\
\object{HIP~56280} &$5.637\pm0.004$&$5.734\pm0.003$&$0.533\pm0.008$&$0.523\pm0.007$&$ 37.44\pm1.15$&$ 3.50\pm0.07$&$3.59\pm0.07$& 1.23 & 1.21 &  9.5 & 253 \\
\object{HIP~58298} &$8.173\pm0.008$&$8.288\pm0.009$&$0.467\pm0.035$&$0.503\pm0.037$&$ 13.52\pm1.74$&$ 3.69\pm0.28$&$3.80\pm0.28$& 1.03 & 1.02 &  4.0 & 316 \\
\object{HIP~58813/15} &$8.029\pm0.010$&$8.718\pm0.014$&$0.634\pm0.017$&$0.726\pm0.024$&$ 18.73\pm1.88$&$ 4.31\pm0.22$&$5.00\pm0.22$& 1.11 & 0.99 & 23.2 &1287 \\
\object{HIP~58862/64} &$9.155\pm0.009$&$9.826\pm0.014$&$0.449\pm0.025$&$0.626\pm0.051$&$  7.99\pm2.47$&$ 2.49\pm0.69$&$3.16\pm0.69$& 1.08 & 1.00 & 27.6 &5933 \\
\object{HIP~59743} &$7.960\pm0.005$&$8.234\pm0.007$&$0.793\pm0.021$&$0.830\pm0.034$&$ 27.50\pm1.54$&$ 5.13\pm0.12$&$5.41\pm0.12$& 0.92 & 0.88 &  7.0 & 256 \\
\object{HIP~62596} &$8.765\pm0.011$&$8.784\pm0.011$&$0.554\pm0.030$&$0.561\pm0.030$&$ 13.51\pm2.75$&$ 4.02\pm0.45$&$4.04\pm0.45$& 1.18 & 1.20 &  9.0 & 800 \\
\object{HIP~64030} &$7.528\pm0.004$&$8.095\pm0.007$&$0.439\pm0.013$&$0.539\pm0.024$&$ 13.24\pm1.99$&$ 2.94\pm0.33$&$3.51\pm0.33$& 1.11 & 1.00 &  7.0 & 580 \\
\object{HIP~65176} &$7.778\pm0.004$&$8.559\pm0.010$&$0.543\pm0.013$&$0.686\pm0.029$&$ 18.86\pm1.49$&$ 4.11\pm0.17$&$4.89\pm0.17$& 1.21 & 1.07 &  5.0 & 272 \\
\object{HIP~65352/55} &$7.213\pm0.004$&$7.345\pm0.004$&$             $&$0.873\pm0.013$&$ 61.76\pm1.24$&$ 6.16\pm0.04$&$6.30\pm0.04$& 0.78 & 0.75 & 26.3 & 427 \\
\object{HIP~69328} &$8.376\pm0.005$&$8.795\pm0.007$&$0.580\pm0.024$&$0.643\pm0.030$&$ 15.37\pm2.60$&$ 4.05\pm0.37$&$4.47\pm0.37$& 0.99 & 0.94 &  6.6 & 487 \\
\object{HIP~70269} &$7.554\pm0.006$&$7.669\pm0.006$&$0.564\pm0.023$&$             $&$ 22.81\pm1.89$&$ 4.39\pm0.18$&$4.41\pm0.18$& 1.01 & 1.01 &  5.8 & 260 \\
\object{HIP~70386} &$7.423\pm0.006$&$7.612\pm0.006$&$0.539\pm0.016$&$0.604\pm0.017$&$ 27.90\pm2.00$&$ 4.61\pm0.16$&$4.80\pm0.16$& 1.13 & 1.01 &  9.3 & 340 \\
\object{HIP~73674} &$8.398\pm0.011$&$8.418\pm0.012$&$0.612\pm0.028$&$0.610\pm0.038$&$ 21.13\pm1.74$&$ 4.97\pm0.18$&$4.99\pm0.18$& 0.95 & 0.93 &  7.4 & 360 \\
\object{HIP~74432/34} &$6.656\pm0.006$&$7.500\pm0.009$&$0.694\pm0.010$&$0.752\pm0.016$&$ 34.20\pm1.78$&$ 4.30\pm0.11$&$5.15\pm0.11$& 0.97 & 0.90 & 23.5 & 693 \\
\object{HIP~76446} &$8.669\pm0.007$&$9.870\pm0.017$&$0.525\pm0.051$&$0.759\pm0.097$&$ 16.50\pm1.81$&$ 4.66\pm0.24$&$5.86\pm0.24$& 1.03 & 0.86 &  7.9 & 498 \\
\object{HIP~76603/02} &$6.466\pm0.008$&$6.555\pm0.007$&$0.483\pm0.014$&$0.515\pm0.013$&$ 41.68\pm2.87$&$ 4.53\pm0.15$&$4.62\pm0.15$& 1.10 & 1.13 & 11.8 & 287 \\
\object{HIP~78024} &$6.983\pm0.004$&$8.621\pm0.014$&$0.553\pm0.012$&$0.823\pm0.044$&$ 26.54\pm1.08$&$ 4.09\pm0.09$&$5.73\pm0.09$& 1.19 & 0.93 &  6.0 & 227 \\
\object{HIP~79818} &$8.507\pm0.006$&$9.118\pm0.012$&$0.480\pm0.025$&$0.577\pm0.067$&$ 10.83\pm2.51$&$ 3.13\pm0.51$&$3.74\pm0.51$& 1.06 & 1.00 &  4.9 & 583 \\
\object{HIP~80399} &$5.970\pm0.004$&$6.733\pm0.008$&$             $&$             $&$ 31.82\pm1.12$&$ 3.47\pm0.08$&$4.24\pm0.08$& 1.24 & 1.09 &  4.7 & 147 \\
\object{HIP~84405} &$5.045\pm0.005$&$5.212\pm0.007$&$0.877\pm0.021$&$             $&$167.08\pm1.07$&$ 6.16\pm0.01$&$6.33\pm0.02$& 0.78 & 0.78 &  4.7 &  28 \\
\object{HIP~ 101292} &$8.459\pm0.006$&$8.479\pm0.007$&$             $&$             $&$ 20.99\pm2.06$&$ 4.99\pm0.21$&$5.01\pm0.21$& 0.98 & 0.98 &  4.0 & 199 \\
\object{HIP~ 103438} &$8.448\pm0.006$&$9.030\pm0.009$&$0.603\pm0.028$&$0.761\pm0.048$&$ 19.63\pm1.87$&$ 4.84\pm0.21$&$5.42\pm0.21$& 1.06 & 0.90 &  4.5 & 235 \\
\object{HIP~ 104687} &$8.144\pm0.006$&$8.189\pm0.006$&$0.638\pm0.056$&$0.714\pm0.060$&$ 20.87\pm1.99$&$ 4.67\pm0.21$&$4.71\pm0.21$& 1.06 & 1.05 &  4.0 & 198 \\
\object{HIP~ 114914} &$8.174\pm0.006$&$8.547\pm0.008$&$0.638\pm0.029$&$0.710\pm0.044$&$ 18.30\pm1.97$&$ 4.39\pm0.23$&$4.76\pm0.23$& 1.09 & 1.04 &  5.3 & 301 \\
         \hline
      \end{tabular}
\end{table}