\documentstyle{article} \def\psnormal{\textwidth=18cm\textheight=21cm \oddsidemargin=-2.0cm\evensidemargin=0cm \topmargin=-1cm \parindent=0cm\parskip=0.3cm} \psnormal \begin{document} \baselineskip=16pt \pagestyle{empty} \footnotesize \vspace{-3.5cm} \footnotesize \begin{table} \caption[ ]{Deconvolution for the Hyades binaries. The photometry is essentially from Johnson \& Knuckles (1955) and the distances from Stern (1994). Spectral types for the primary and secondary components were assigned from (B-V) color indices by using the Schmidt--Kaler's (1982) ZAMS. } \begin{tabular}{llllllllclllcc} \hline Star & \multicolumn{3}{c}{ (B-V)} & Dist. & \multicolumn{3}{c}{M$_{\rm V}$}&V$_{\rm obs}$& \multicolumn{3}{c}{Sp. Type}& Binarity\\ \cline{2-4} \cline{6-8} \cline{10-12} & Obs. & Prim. & Sec. & (pc) & Obs. & Prim. & Sec. & & Obs. & Prim. & Sec. & \\ (1) & (2) & (3) & (4) & (5) & (6) & (7) & (8) & (9)& (10) &(11)& (12) & (13) \\ \hline vB~1$^{(1)}$ & 0.566 & 0.559 &1.448 & 43.1 &4.228 & 4.241 & 9.028 &7.40& -- & F9 V & M1 V & VB \\ V471 Tau$^{(2)}$& 0.85 &$\sim$0.993& -- & 59 & 5.86 & 5.35 & 9.75 &9.71& -- & K2 V & WD & SB1 \\ vB~9 & 0.708 & -- & -- &(47.9)$^{\rm (b)}$&5.27$^{\rm (b)}$& -- & -- &8.67& -- & G6 V & -- & SB1 \\ vB~14 & 0.355 & 0.350 & 1.337& 38.3 & 2.814 & 2.822 & 8.141 &5.73& -- & F2 V & K8 V & SB \\ BD+23$^\circ635^{(3)}$& 1.09 & 1.043 &1.362 &(39.9)$^{\rm (a)}$&6.375 &6.573 & 8.322 &9.38& -- & K3.5 V& K9 V & SB2 \\ vB~162$^{(4)}$ & 0.705 & 0.666 & 0.746& 49.1 & 4.375 & 4.934 & 5.283 &7.83& -- & G4 V & G9 V & SB2 \\ vB~22$^{(5)}$ & 0.771 & 0.713 & 0.945& 50.8 & 4.811 & 5.155 & 6.226 &8.34& G8 V & G6 V & K3 V & SB2 \\ vB~23$^{(6)}$ & 0.679 & 0.654 & 0.714& 49.3 & 4.076 & 4.815 & 5.161 &7.54& -- & G3 V & G6 V & SB2 \\ BD+22$^\circ669^{(7)}$& 0.99 & 0.933 & 1.167&(53.1)$^{\rm (a)}$& 5.859 & 6.190 & 7.310 &9.48& K0 & K2 V & K5 V & SB2 \\ vB~29$^{(8)}$ & 0.561 & 0.520 & 0.670& 47.3 & 3.506 & 3.898 & 4.896 &6.88& F8 V & F8 V & G5 V & SB \\ vB~34$^{(9)}$ & 0.457 & 0.435 & 0.461& 50.3 & 2.662 & 3.456 & 3.506 &6.17& F6 V & F5 V & F6 V & SB2 \\ vB~38$^{(10)}$ & 0.320 & 0.296 & 0.764& 47.6 & 2.332 & 2.402 & 5.350 &5.72& Am & F0 V & G9 V & SB1 \\ vB~40$^{(11)}$ & 0.563 & 0.528 & 1.042& 41.9 & 3.879 & 3.974 & 6.567 &6.99& G9 V & F9 V & K4 V & VB/SB1 \\ vB~39$^{(12)}$ & 0.678 & 0.678 & -- & 38.2 & 4.950 & 4.950 & -- &7.86& -- & G5 V & -- & SB \\ vB~42 & 0.759 & 0.750 & 1.492& 52.0 & 5.280 & 5.298 & 9.750 &8.86& G9 V & G8 V & M2 V & PhB \\ vB~50 & 0.601 & 0.578 & 1.252& 45.9 & 4.311 & 4.361 & 7.668 &7.62& G1 V & G0 V & K6 V & SB \\ vB~52$^{(13)}$ & 0.597 & 0.597 & -- & 43.9 & 4.588 & 4.588 &-- &7.80& G1 V & G0 V & -- & SB? \\ vB~140$^{(14)}$ & 0.757 & 0.708 & 1.134& 51.2 & 4.973 & 5.131 & 7.130 &8.94& -- & G6 V & K5 V & SB2 \\ vB~57$^{(15)}$ & 0.491 & 0.466 & 0.530& 51.2 & 2.914 & 3.542 & 3.989 &6.46& F7 V & F6 V & F8 V & VB/SB2 \\ vB~58$^{(16)}$ & 0.680 & 0.642 & 0.742& 46.1 & 4.211 & 4.771 & 5.269 &7.53& G6 V & G4 V & G8 V & VB/SB2 \\ vB~59 & 0.543 & 0.540 & 1.492& 47.9 & 4.088 & 4.094 & 9.739 &7.49& F8 V & F9 V & M2 V & SB \\ vB~62 & 0.537 & 0.518 & 1.194& 51.0 & 3.842 & 3.883 & 7.443 &7.38& F8 V & F8 V & K5.5 V& SB1 \\ vB~63 & 0.632 & 0.630 & 1.522& 46.6 & 4.718 & 4.721 & 11.074 &8.06& G5 V & G2 V & M3 V & VB/SB1 \\ vB~178$^{(17)}$ & 0.837 & 0.794 & 1.295& 52.7 & 5.421 & 5.541 & 7.868 &9.03& K0 V & K0 V & K6 V & SB? \\ vB~69 & 0.746 & 0.714 & 1.315& 51.5 & 5.081 & 5.159 & 7.983 &8.64& G8 V & G6 V & K7 V & SB1 \\ vB~75$^{(18)}$ & 0.531 & 0.481 & 0.545& 52.0 & 3.010 & 3.644 & 4.136 &6.59& F8 V & F7 V & F9 V & VB/SB3 \\ vB~77 & 0.502 & 0.489 & 1.281& 47.2 & 3.680 & 3.705 & 7.800 &7.05& F7 V & F8 V & K6.5 & SB1 \\ vB~81 & 0.470 & 0.461 & 1.327& 52.7 & 3.491 & 3.507 & 8.068 &7.10& F6 V & F6 V & K7 V & SB \\ vB~181 & 1.167 & 1.122 & 1.426& 49.4 & 6.851 & 7.050 & 8.793 &10.32& K & K5 V & M1 V & PhB \\ vB~182 & 0.884 & 0.820 & 1.062& 53.3 & 5.296 & 5.661 & 6.657 &8.93& -- & K0 V & K4 V & SB1 \\ vA677$^{(19)}$ & 1.23 & 1.23 & -- & 43.6 & 7.833 & 7.833 & -- &11.03&K6 V & K6 V & -- & SB1 \\ vB~91 & 0.883 & 0.819 & 1.074& 53.1 & 5.315 & 5.659 & 6.728 &8.94& K1 V & K0 V & K4 V & VB/SB1 \\ vB~96$^{(20)}$ & 0.841 & 0.811 & 0.881& 50.1 & 5.011 & 5.634 & 5.910 &8.51&KO IV/V& K0 V & K2 V & VB/SB1 \\ J301$^{(21)}$ & 1.085 & 1.085 & -- & 16.7 & 7.306 & 6.789 & -- &8.42&dK5e & K4 V & -- & SB1 \\ vB~102 & 0.603 & 0.576 & 1.190& 44.7 & 4.288 & 4.351 & 7.411 &7.54& G1 V & G0 V & K5.5 V& VB/SB1 \\ J304$^{(22)}$ & 1.15 & 1.109 & 1.451&(47.1)$^{\rm (a)}$& 6.805 & 6.965 & 8.963 &10.17& K5 & K5 V & M1 V & SB1 \\ vB~106 & 0.669 & 0.623 & 1.089& 48.6 & 4.527 & 4.666 & 6.829 &7.96& -- & G1 V & K4 V & SB1 \\ vB~185$^{(23)}$ & 1.1 & 1.046 & 1.299& 51.6 & 5.907 & 6.587 & 7.886 &9.47& K3 V & K3 V & K7 V & SB2 \\ vB~142 & 0.665 & 0.661 & 1.501& 50.3 & 4.832 & 4.832 &10.304 &8.34& -- & G4 V & M2 V & SB1 \\ vB~113$^{(24)}$ & 0.549 & 0.549 & -- & 41.2 & 4.186 & 4.186 & -- &7.26& -- & F9 V & -- & SB1 \\ vB~114 & 0.723 & 0.706 & 1.435& 49.0 & 5.089 & 5.124 & 8.845 &8.54& -- & G6 V & M1 V & SB1 \\ J331$^{(25)}$ & 1.41 & 1.400 & 1.421&(43.3)$^{\rm (a)}$& 7.938 & 8.616 & 8.767 &11.12& -- & K8.8 V& K9.2 V& SB2 \\ vB~115 & 0.843 & 0.814 & 1.393& 50.5 & 5.574 & 5.645 & 8.567 &9.09& -- & K0 V & M0 V & SB1 \\ vB~117$^{(26)}$ & 1.06 & 1.036 & 1.093& 48.02 & 6.263 & 6.544 & 6.853 &9.67& K3 V & K3 V & K3 V & SB2 \\ vB~119 & 0.559 & 0.528 & 1.077& 44.3 & 3.888 & 3.969 & 6.745 &7.12& -- & F9 V & K4 V & SB1 \\ vB~120$^{(27)}$ & 0.735 & 0.712 & 0.764& 52.7 & 4.494 & 5.150 & 5.350 &7.71& -- & G6 V & G8 V & VB/SB2 \\ vB~121 & 0.504 & 0.493 & 1.324& 52.1 & 3.706 & 3.726 & 8.044 &7.29& -- & F8 V & K7 V & SB \\ vB~122$^{(28)}$ & 0.541 & 0.531 & 0.553& 52.0 & 3.346 & 4.009 & 4.198 &6.76& -- & F9 V & F9 V & VB/SB2 \\ vB~124$^{(29)}$ & 0.497 & 0.428 & 0.783& 54.2 & 3.057 & 3.319 & 4.879 &6.27& F5/G8& F5 V & G5 V & SB2 \\ \hline \end{tabular} \end{table} $^{\rm (a)}$ Distance estimated from the photometry. \\ $^{\rm (b)}$ Calculated from V and ${\rm _{\rm binary}}$=3.40\\ $^{(1)}$ ADS~2451. The photometry include the visual companion. Mason et al. (1993) estimated $\Delta$V=6.0$^{\rm m}$.\\ $^{(2)}$ Distance and spectral types from Strassmeier et al 1993. (B-V)$_{\rm p}$ was assigned according the espectral type.\\ $^{(3)}$ $\Delta$V=1.75$^{\rm m}$ from Griffin \& Gunn (1981). Probable triple system.\\ $^{(4)}$ $\Delta$V=0.5$^{\rm m}$ from Griffin \& Gunn (1981).\\ $^{(5)}$ (B-V)$_{\rm p}$ measured directly during the eclipse (Schiller \& Milone 1987).\\ $^{(6)}$ $\Delta$V=0.35$^{\rm m}$ from Batten \& Wallerstein (1973). It could have an additional component.\\ $^{(7)}$ $\Delta$V=1.12$^{\rm m}$ from Griffin et al. (1982).\\ $^{(8)}$ ADS~3135. $\Delta$V=1.0$^{\rm m}$ from Wickes (1975). V=\{7.24+8.24\} from Peterson \& Solenski (1987). Visual companion included in the photometry.\\ $^{(9)}$ Boesgaard \& Tripicco (1986) obtained $\Delta$V=0.056$^{\rm m}$ from the ratio between spectral lines.\\ $^{(10)}$ Visual component included in the photometry.\\ $^{(11)}$ ADS~3169. Visual component included in the photometry.\\ $^{(12)}$ The contribution from the secondary is apparently negligible.\\ $^{(13)}$ The contribution from the secondary is apparently negligible.\\ $^{(14)}$ $\Delta$V=2.0$^{\rm m}$ from Griffin et al. (1985). \\ $^{(15)}$ $\Delta$V=0.45$^{\rm m}$ from Peterson \& Solenski (1987). V=\{7.01+7.46\}. The visual companion is included in the photometry.\\ $^{(16)}$ ADS~3210. $\Delta$V=0.50$^{\rm m}$ from Heintz (1969). V=\{8.06+8.56\} from Peterson \& Solenski (1987). The visual companion is included in the photometry.\\ $^{(17)}$ V$_{\rm obs}$=9.03 from Mermilliod (1976).\\ $^{(18)}$ ADS~3248. $\Delta$V=0.65$^{\rm m}$ from Dombrowski (1991). Triple system. The inner pair is the SB2.\\ \indent The whole deconvolution is \{F7 V + K0 V\} + F9 V, V = \{3.644 + 5.655\} + 4.136, (B-V) = \{0.481 + 0.819\} + 0.545\\ $^{(19)}$ The contribution from the secondary is apparently negligible.\\ $^{(20)}$ The visual companion is {\it not} included in the photometry.\\ $^{(21)}$ Strassmeier et al. (1993) give M$_{\rm V}=6.8^{\rm m}$, D=16.7 pc and dK5e. Apparent magnitude from Eggen \& Greenstein (1965). Distance from Borgman \& Lippicott (1983). Another possibility for the deconvolution could be (B-V)$_{\rm calc}$=1.085, (B-V)$_{\rm p}$=1.068, (B-V)$_{\rm s}$=1.7, M$_{\rm calc}$=6.648, M$_{\rm p}$=6.687, M$_{\rm s}$=10.291, (1+$\alpha$)=1.036, $\Delta$V=3.6$^{\rm m}$.\\ $^{(22)}$ $\Delta$V=2.0, Griffin et al. (1985).\\ $^{(23)}$ The deconvolution was taken from Griffin et al. (1985). \\ $^{(24)}$ The contribution from the secondary is apparently negligible.\\ $^{(25)}$ $\Delta$V=0.14$^{\rm m}$, Spectral types, distance and deconvolution from Griffin et al. (1985).\\ $^{(26)}$ V$_{\rm primary}$=10.28, V$_{\rm secondary}$=10.59, Griffin \& Gunn (1978). Distance from Schwan (1991), Spectral types from Strassmeier et al. (1993)\\ $^{(27)}$ $\Delta$V=0.2$^{\rm m}$ from Thorburn et al. (1993) from the ratio between Ca{\sc I} 6718\AA. V$_{\rm obs}$=7.34, 7.59, 7.71, 7.73 and 8.18, from Schwan (1991), Mermilliod (1976), Stern (1994) and Mason et al. (1993), respectively.\\ $^{(28)}$ ADS~3475. Also (B-V)$_{\rm obs}$=0.50 from Mermilliod (1976). $\Delta$V=0.19$^{\rm m}$ from Dombrowski (1991). The visual component is included in the photometry. \\ $^{(29)}$ ADS~3483. Triple system (Griffin et al. 1985):\\ \indent \{F5 V + G8 V\} + G4 V, V = \{3.4 + 5.58\} + 4.96, (B-V) = \{0.42 + 0.81\} + 0.68\\ \end{document}