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\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 ${\rm <m-M>_{\rm binary}}$=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}
