Table 1: 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. As discussed in the text, the formal errors on magnitudes and colors are likely underestimated.
Object VA VB (B-V)A (B-V)B $\pi$ MV(A) MV(B) MA MB $\rho$ $\rho$
          mas     $M_{\odot}$ $M_{\odot}$ '' AU
HD 8009 $8.819\pm0.007$ $9.724\pm0.017$ $0.64\pm0.03$ $0.82\pm0.07$ 15.43 $\pm$ 2.02 4.61 $\pm$ 0.29 5.52 $\pm$ 0.29 0.95 0.85 4.7 326
HD 8071 $7.312\pm0.003$ $7.573\pm0.004$ $0.58\pm0.01$ $0.60\pm0.01$ 19.67 $\pm$ 1.58 3.73 $\pm$ 0.17 3.99 $\pm$ 0.17 1.25 1.22 2.2 115
HD 9911 $9.428\pm0.008$ $9.448\pm0.008$ $0.90\pm0.04$ $0.89\pm0.04$ 20.40 $\pm$ 3.32 5.74 $\pm$ 0.36 5.76 $\pm$ 0.36 0.85 0.85 3.9 213
HD 13357 $8.180\pm0.006$ $8.647\pm0.010$ $0.67\pm0.03$ $0.73\pm0.05$ 20.41 $\pm$ 1.75 4.67 $\pm$ 0.19 5.14 $\pm$ 0.19 0.98 0.93 5.9 297
HD 17159 $8.775\pm0.007$ $8.923\pm0.007$ $0.54\pm0.03$ $0.53\pm0.03$ 14.65 $\pm$ 2.24 4.40 $\pm$ 0.33 4.55 $\pm$ 0.33 1.15 1.12 2.7 203
HD 19440 $7.874\pm0.004$ $8.574\pm0.007$ $0.47\pm0.01$ $0.53\pm0.02$ 12.55 $\pm$ 1.39 3.27 $\pm$ 0.24 3.96 $\pm$ 0.24 1.25 1.14 6.0 501
HD 30101 $8.782\pm0.009$ $8.848\pm0.009$ $0.82\pm0.04$ $0.91\pm0.03$ 23.43 $\pm$ 2.55 5.53 $\pm$ 0.24 5.66 $\pm$ 0.24 0.84 0.83 4.6 205
HD 33334 $8.023\pm0.004$ $8.857\pm0.009$ $0.70\pm0.03$ $0.80\pm0.07$ 21.39 $\pm$ 2.18 4.59 $\pm$ 0.22 5.42 $\pm$ 0.22 1.00 0.89 4.7 229
HD 66491 $9.253\pm0.009$ $9.312\pm0.009$ $0.75\pm0.05$ $0.67\pm0.05$ 15.11 $\pm$ 2.71 4.85 $\pm$ 0.39 4.91 $\pm$ 0.39 0.96 0.96 5.1 387
BD+23 1978 $9.395\pm0.010$ $9.530\pm0.011$ $0.80\pm0.06$ $0.75\pm0.05$ 24.04 $\pm$ 2.97 6.17 $\pm$ 0.27 6.31 $\pm$ 0.27 0.84 0.84 2.6 115
HD 106515 $7.960\pm0.005$ $8.234\pm0.007$ $0.79\pm0.02$ $0.83\pm0.03$ 27.50 $\pm$ 1.54 5.13 $\pm$ 0.12 5.41 $\pm$ 0.12 0.93 0.89 7.0 257
HD 108574/5 $7.418\pm0.005$ $7.972\pm0.007$ $0.56\pm0.01$ $0.67\pm0.02$ 25.06 $\pm$ 1.81 4.37 $\pm$ 0.16 4.93 $\pm$ 0.16 1.22 1.11 9.8 399
HD 123963 $8.758\pm0.006$ $9.511\pm0.010$ $0.60\pm0.03$ $0.54\pm0.04$ 13.81 $\pm$ 1.74 4.33 $\pm$ 0.28 5.08 $\pm$ 0.28 1.08 0.96 2.6 200
HD 132563 $8.966\pm0.007$ $9.472\pm0.010$ $0.54\pm0.03$ $0.57\pm0.05$ 10.15 $\pm$ 2.01 3.62 $\pm$ 0.44 4.13 $\pm$ 0.44 1.13 1.06 4.2 491
HD 132844 $9.022\pm0.006$ $9.114\pm0.007$ $0.55\pm0.05$ $0.63\pm0.05$ 16.57 $\pm$ 2.05 4.99 $\pm$ 0.27 5.08 $\pm$ 0.27 1.01 0.99 3.0 192
HD 135101 $6.656\pm0.006$ $7.500\pm0.009$ $0.69\pm0.01$ $0.75\pm0.02$ 34.18 $\pm$ 1.78 4.30 $\pm$ 0.11 5.15 $\pm$ 0.11 0.97 0.95 23.5 694
HD 190042 $8.755\pm0.009$ $8.778\pm0.006$ $0.73\pm0.03$ $0.80\pm0.04$ 16.52 $\pm$ 1.64 4.76 $\pm$ 0.22 4.79 $\pm$ 0.22 0.96 0.94 4.2 264
HD 200466 $8.399\pm0.005$ $8.528\pm0.006$ $0.71\pm0.02$ $0.79\pm0.03$ 22.83 $\pm$ 1.75 5.14 $\pm$ 0.17 5.28 $\pm$ 0.17 0.99 0.97 4.7 210
HIP 104687 $8.144\pm0.006$ $8.189\pm0.006$ $0.64\pm0.06$ $0.71\pm0.06$ 20.87 $\pm$ 1.99 4.67 $\pm$ 0.21 4.72 $\pm$ 0.21 1.09 1.08 4.0 198
HD 213013 $8.982\pm0.008$ $9.612\pm0.013$ $0.81\pm0.04$ $0.93\pm0.08$ 21.59 $\pm$ 2.01 5.58 $\pm$ 0.20 6.21 $\pm$ 0.20 0.93 0.84 5.5 263
HD 215812 $7.275\pm0.005$ $7.576\pm0.006$ $0.64\pm0.02$ $0.70\pm0.02$ 31.94 $\pm$ 1.66 4.78 $\pm$ 0.11 5.08 $\pm$ 0.11 0.95 0.92 2.2 70
HD 216122 $8.062\pm0.011$ $8.186\pm0.013$ $0.58\pm0.02$ $0.58\pm0.03$ 13.11 $\pm$ 2.36 3.35 $\pm$ 0.40 3.47 $\pm$ 0.40 1.23 1.22 5.3 464
HD 219542 $8.174\pm0.006$ $8.547\pm0.008$ $0.64\pm0.03$ $0.71\pm0.04$ 18.30 $\pm$ 1.97 4.39 $\pm$ 0.23 4.78 $\pm$ 0.23 1.08 1.05 5.3 303


Source LaTeX | All tables | In the text