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{\bf Table 1.} Catalogue of 22 standard stars observed and transformed 
to the Crawford-Barnes {\em uvby} and the Crawford-Mander H$\beta$ 
standard systems. The internal rms errors of one observation are given 
in columns 8 to 12 in units of 0.001 mag. Columns 13 to 17 give the 
difference D = standard value minus transformed value, in units of 0.001 
mag. N is the number of measures.
\footnotesize
\begin{tabular}{lrrrrrrcccccrrrrr}
\hline
Star & $V$ & $(b-y)$ & $m_{1}$ & $c_{1}$ & $\beta$ & N & & & $\sigma$ & & &
 & & D & & \\
 & & & & & & & $V$ & $(b-y)$ & $m_{1}$ & $c_{1}$ & $\beta$ & 
$V$ & $(b-y)$ & $m_{1}$ & $c_{1}$ & $\beta$ \\
\hline
 & & & & & & & & & & & & & & & & \\
HR 63 &4.616 &0.019 &0.192 &1.031 &2.885 &3 &009 &004 &002 &013 &010 &
002 &007 &--012 &018 &--005 \\
BD +56$^{\circ}$ 510 &9.339 &0.281 &--0.054 &0.149 &2.615 &11 &006 &007 &009 
&012 &017 & --019 &--004 &004 &017 &004 \\
HD 14434 &8.497 &0.191 &--0.023 &--0.088 &2.576 &23 &006 &006 &009 &012 
&008 &003 &--010 &006 &--006 &006 \\
BD +56$^{\circ}$ 576 &9.388 &0.292 &--0.073 &0.153 &2.630 &2 &004 &003 
&001 &001 &005 &--008 &--010 &009 &007 &--009 \\
HD 14476 &8.753 &0.359 &--0.103 &0.109 &2.598 &21 &010 &011 &012 &011 &008 &
--003 &--008 &009 &--001 &002 \\
 & & & & & & & & & & & & & & & & \\
HD 21092 &8.498 &0.108 &0.199 &0.943 &2.891 &3 &005 &003 &004 &004 &010 &
--018 &000 &004 &013 &011 \\
HD 21239 &7.949 &0.063 &0.184 &0.999 &2.911 &3 &008 &004 &006 &002 &012 &
--001 &--002 &--001 &003 & --003 \\
HD 21398 &7.372 &0.018 &0.132 &0.837 &2.845 &4 &010 &003 &007 &006 &004 &
--012 &003 &--006 &--006 &--017 \\
HR 1140 &5.456 &0.001 &0.101 &0.634 &2.747 &8 &008 &006 &008 &017 &003 &
005 &004 &--004 &016 &003 \\
HR 1144 &5.659 &--0.018 &0.099 &0.633 &2.745 &8 &004 &002 &005 &010 &004 &
006 &--003 &008 &005 &005 \\
 & & & & & & & & & & & & & & & & \\
HR 1672 &5.416 &0.131 &0.252 &0.822 &2.830 &1 &-- &-- &-- &-- &-- &
008 &005 &--001 &013 &--002 \\
HR 1861 &5.326 &--0.072 &0.067 &0.003 &2.617 &2 &001 &001 &003 &001 &004 &
015 &--002 &006 &--001 &--002 \\
HR 2886 &5.282 &0.038 &0.135 &0.167 &2.849 &2 &016 &008 &008 &018 &004 &
--005 &--001 &008 &011 &-- \\
HR 4119 &5.070 &--0.060 &0.109 &0.487 &2.722 &2 &006 &006 &008 &006 &005 &
011 &--001 &004 &--008 &008 \\
HR 4378 &6.662 &0.024 &0.187 &1.063 &2.903 &3 &015 &005 &007 &007 &005 &
--002 & 000 &003 &--011 &-- \\
 & & & & & & & & & & & & & & & & \\
HR 4705 &6.194 &--0.011 &0.180 &1.029 &2.899 &2 &009 &007 &006 &007 &005 &
006 &009 &--011 &005 &-- \\
HR 7858 &5.403 &0.019 &0.210 &0.935 &2.916 &3 &018 &005 &004 &039 &003 &
--005 &004 &--003 &048 &002 \\
HR 8622 &4.906 &--0.068 &0.049 &--0.125 &2.597 &3 &016 &008 &011 &005 &003 &
--017 &002 &--012 &008 &--010 \\
BD +61$^{\circ}$ 2350 &9.204 &0.602 &--0.172 &0.150 &2.633 &5 &012 &004 
&009 &005 &007 & 006 &003 &--006 &--001 &--007 \\
HD 216532 &8.020 &0.478 &--0.143 &0.018 &2.617 &3 &014 &003 &005 &014 &006 &
010 &001 &--001 &009 &--001 \\
 & & & & & & & & & & & & & & & & \\
HD 217035 &7.758 &0.414 &--0.117 &0.007 &2.616 &5 &012 &001 &005 &014 &006 &
002 &002 &002 &--003 &004 \\
HD 217086 &7.662 &0.530 &--0.158 &--0.001 &2.607 &4 &008 &003 &003 &011 &003 &
--002 &001 &000 &000 &--016 \\
 & & & & & & & & & & & & & & & & \\
\hline
\end{tabular}

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{\bf Table 5.} Photometric data for Be stars in h and $\chi$ Per. Column 
1 is the star number as given by Oosterhoff (1937). Column 2 is the HD 
or BD number. Columns 3 to 7 give the photometric magnitude, colour and 
indices, and columns 8 to 12 the internal rms error of each value. 
Column 13 gives the number of individual measurements, and column 14 
the reference in which the star has been classified as Be. Probable nonmembers
are identified with an asterisk in the Ref. column.

\begin{tabular}{lrrrrrrrrrrrrr}
\hline
 Star & HD/BD & $V$ & $b-y$ & $m_{1}$ & $c_{1}$ & $\beta$ & $\sigma_{V}$ & 
$\sigma_{b-y}$ &
 $\sigma_{m_{1}}$ & $\sigma_{c_{1}}$ & $\sigma_{\beta}$ & N & Ref. \\
\hline
 & & & & & & & & & & & & & \\
    49  & +56$^{\circ}$ 473   &   9.135 &   0.317 &  -0.106 &  -0.005 &   
2.451 & 0.032 & 0.007 &   0.009 &   0.006 &   0.010 & 2 & 1\\
    146 & 13900               &   9.181 &   0.199 &  -0.030 &  0.090  &   
2.599 & 0.003 & 0.015 &   0.021 &   0.023 &   0.005 & 2 & 2,*\\   
    309 & +56$^{\circ}$ 484   &   9.431 &   0.339 &  -0.095 &  -0.052 &   
2.451 & 0.004 & 0.006 &   0.013 &   0.032 &   0.002 & 2 & 3\\
    566 & +56$^{\circ}$ 493   &   9.675 &   0.197 &  -0.018 &  0.107  &   
2.603 & 0.007 & 0.005 &   0.004 &   0.008 &   0.002 & 2 & 1,*\\   
    717 & +56$^{\circ}$ 502   &   9.283 &   0.283 &  -0.058 &   0.106 &   
2.580 & 0.004 & 0.009 &   0.015 &   0.006 &   0.005 & 2 & 4\\
    847 & +56$^{\circ}$ 511   &   9.119 &   0.348 &  -0.095 &   0.150 &   
2.573 & 0.007 & 0.003 &   0.009 &   0.016 &   0.007 & 3 & 1\\
   1161 & +56$^{\circ}$ 529   &  10.201 &   0.391 &  -0.090 &   0.132 &   
2.545 & 0.020 & 0.005 &   0.005 &   0.027 &   0.011 & 3 & 5\\
   1261 & +56$^{\circ}$ 534   &   9.593 &   0.444 &  -0.102 &  -0.002 &   
2.394 & 0.006 & 0.012 &   0.064 &   0.017 &   0.004 & 3 & 3\\
   1268 &  14162              &   9.390 &   0.354 &  -0.081 &   0.125 &   
2.600 & 0.012 & 0.008 &   0.022 &   0.036 &   0.006 & 3 & 6\\
   1282 &                     &  11.045 &   0.456 &  -0.114 &   0.216 &   
2.533 & 0.009 & 0.012 &   0.022 &   0.010 &   0.031 & 3 & 7\\
   1702 & +56$^{\circ}$ 548   &   9.714 &   0.320 &  -0.077 &   0.081 &   
2.503 & 0.012 & 0.007 &   0.011 &   0.012 &   0.013 & 2 & 8\\
   1926 & +56$^{\circ}$ 559   &   9.929 &   0.418 &  -0.135 &  -0.043 &   
2.422 & 0.021 & 0.002 &   0.009 &   0.026 &   0.003 & 2 & 9\\
   1977 &                     &  12.268 &   0.355 &  -0.088 &   0.285 &   
2.488 & -     &  -    &   -     &   -     &   -     & 1 & 6\\
   2088 & +56$^{\circ}$ 563   &  11.153 &   0.355 &  -0.185 &   0.312 &   
2.592 & -     &  -    &   -     &   -     &   -     & 1 & 9\\
   2091 &                     &  11.770 &   0.349 &  -0.096 &   0.385 &   
2.586 & 0.083 & 0.023 &   0.024 &   0.038 &   0.022 & 2 & 6\\
   2138 & 14422               &   9.290 &   0.381 &  -0.107 &   0.092 &   
2.549 & 0.022 & 0.008 &   0.005 &   0.000 &   0.010 & 2 & 9\\
   2165 & +56$^{\circ}$ 566   &   9.999 &   0.380 &  -0.133 &  -0.003 &   
2.477 & 0.035 & 0.019 &   0.029 &   0.016 &   0.008 & 3 & 9\\
   2242 &                     &  11.091 &   0.327 &  -0.092 &   0.361 &   
2.546 & 0.031 & 0.005 &   0.006 &   0.015 &   0.002 & 2 & 5\\
   2262 &                     &  10.606 &   0.337 &  -0.105 &   0.200 &   
2.634 & 0.008 & 0.003 &   0.010 &   0.000 &   0.001 & 2 & 9\\
   2284 & +56$^{\circ}$ 573   &   9.696 &   0.357 &  -0.096 &  -0.017 &   
2.391 & 0.008 & 0.010 &   0.016 &   0.015 &   0.021 & 3 & 9\\
   2371 & +56$^{\circ}$ 578   &   9.228 &   0.304 &  -0.070 &   0.121 &   
2.595 & 0.025 & 0.006 &   0.007 &   0.016 &   0.008 & 3 & 10\\
   2402 & +56$^{\circ}$ 582   &   9.534 &   0.487 &  -0.138 &   0.104 &   
2.525 & 0.015 & 0.006 &   0.002 &   0.021 &   0.006 & 3 & 9\\
   2563 &                     &  10.557 &   0.372 &  -0.102 &   0.007 &   
2.464 & 0.005 & 0.003 &   0.011 &   0.020 &   0.003 & 2 & 8\\
   2566 &                     &  10.520 &   0.387 &  -0.081 &   0.153 &   
2.496 & -     & -     &   -     &   -     &   -     & 1 & 11\\
   2649 &                     &  10.349 &   0.309 &  -0.089 &   0.183 &   
2.540 & 0.003 & 0.010 &   0.009 &   0.011 &   0.008 & 2 & 6\\
   2759 &                     &  10.990 &   0.514 &  -0.152 &   0.107 &   
2.485 & 0.009 & 0.000 &   0.005 &   0.003 &   0.004 & 2 & 7\\
   2771 &                     &  11.203 &   0.473 &  -0.125 &   0.208 &   
2.553 & 0.031 & 0.011 &   0.004 &   0.005 &   0.013 & 2 & 7\\
   2804 &                     &  10.456 &   0.375 &  -0.093 &   0.059 &   
2.543 & 0.052 & 0.016 &   0.023 &   0.017 &   0.033 & 2 & 12\\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

\begin{tabular}{ll}
 & \\
1.- Wackerling (1970)                  & 7.- Slettebak (1985) \\
2.- Hardorp {\em et al.}, (1965)       & 8.- Merrill \& Burwell (1943) \\
3.- Slettebak (1968)                   & 9.- Merrill \& Burwell (1933) \\
4.- Fabregat {\em et al.}, (1994b)     & 10.- Schild (1965) \\
5.- Schild \& Romanishin (1976)        & 11.- Merrill \& Burwell (1949) \\
6.- Gonz\'{a}lez \& Gonz\'{a}lez (1954)& 12.- Sanduleak \& Bidelman (1980) \\
\end{tabular}

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{\bf Table 6.} Photometric data for Be stars in NGC 663. Columns as in 
Table 5. Cluster numbers are from Wallenquist (1929).

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
Star & HD/BD & $V$  & $b-y$  & $m_{1}$ & $c_{1}$ & $\beta$ & $\sigma_{V}$  &
    $\sigma_{b-y}$ & $\sigma_{m_{1}}$ & $\sigma_{c_{1}}$ & 
$\sigma_{\beta}$&N & Ref.\\
\hline        
 & & & & & & & & & & & & & \\
  2 &    &  12.299 &   0.566 &  -0.145 &   0.159 &   2.512 &         &
             &         &         &         & 1 & 1\\
  6 &    &  12.100 &   0.583 &  -0.214 &   0.183 &   2.581 &         &
             &         &         &         & 1 & 2\\
  8 &    &  12.205 &   0.574 &  -0.166 &   0.439 &   2.720 &         &
             &         &         &         & 1 & 1\\
 10 &    &  11.946 &   0.536 &  -0.145 &   0.159 &   2.598 &         &
             &         &         &         & 1 & 1\\
 21 &    &  10.624 &   0.506 &  -0.143 &   0.221 &   2.571 &   0.014 &
       0.002 &   0.008 &   0.007 &   0.009 & 2 & 3\\
 57 &    &  13.278 &   0.548 &  -0.122 &   0.626 &   2.626 &         &
             &         &         &         & 1 & 4\\
 84 &    &  13.885 &   0.579 &  -0.127 &   0.470 &   2.510 &         &
             &         &         &         & 1 & 4\\
 93 &    &  12.016 &   0.541 &  -0.173 &   0.233 &   2.486 &         &
             &         &         &         & 1 & 1\\
107 &+60$^{\circ}$ 340  &  10.233 &   0.473 &  -0.121 &   0.302 &   2.633 &    
&            &         &         &         & 1 & 5\\
110 &+60$^{\circ}$ 344  &  10.103 &   0.469 &  -0.104 &   0.288 &   2.601 &    
&            &         &         &         & 1 & 3\\
130 &    &  12.492 &   0.596 &  -0.195 &   0.347 &   2.513 &         &
             &         &         &         & 1 & 1\\
141 &+60$^{\circ}$ 341  &  10.711 &   0.511 &  -0.150 &   0.148 &   2.421 &    
&            &         &         &         & 1 & 6\\
194 &    &  11.331 &   0.600 &  -0.229 &   0.118 &   2.496 &         &
             &         &         &         & 1 & 1\\
222 &    &  11.390 &   0.568 &  -0.181 &   0.030 &   2.537 &         &
             &         &         &         & 1 & 1\\
243 &+60$^{\circ}$ 325  &  9.855  &   0.430 &  -0.123 &   0.305 &   2.574 &    
&            &         &         &         & 1 & 7\\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

\begin{tabular}{ll}
 & \\
1.- Gonz\'{a}lez \& Gonz\'{a}lez (1954) & 5.- Merrill \& Burwell (1949) \\
2.- Coyne {\em et al.} (1978)           & 6.- Dolidze (1975) \\
3.- Schild \& Romanishin (1976)         & 7.- Merrill \& Burwell (1943) \\
4.- Sanduleak (1990)                    & \\
\end{tabular}

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{\bf Table 7.} Photometric data for Be stars in Pleiades. Columns as in 
Table 5. Cluster numbers are from Hertzsprung (1947).

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
 Star & HD & $V$ & $b-y$ & $m_{1}$ & $c_{1}$ & $\beta$  & $\sigma_{V}$    &
    $\sigma_{b-y}$ & $\sigma_{m_{1}}$& $\sigma_{c_{1}}$& 
$\sigma_{\beta}$ & N & Ref.\\
\hline
 & & & & & & & & & & & & & \\
 468 & 23302 &  3.727 &  -0.038 &   0.094 &   0.618 &   2.704 &         &
             &         &         &         & 1 & 1\\
 980 & 23480 &  4.174 &   0.011 &   0.075 &   0.549 &   2.615 &   0.003 &
       0.001 &   0.004 &   0.005 &   0.001 & 2 & 2\\
1432 & 23630 &  2.919 &  -0.028 &   0.096 &   0.626 &   2.661 &         &
             &         &         &         & 1 & 1\\
2181 & 23862 &  5.042 &  -0.015 &   0.082 &   0.634 &   2.578 &   0.010 &
       0.001 &   0.002 &   0.000 &   0.003 & 2 & 1\\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

1.- Merrill \& Burwell (1933) \\
2.- Wakerling (1970) \\ 

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{\bf Table 8.} Photometric data for Be stars in the $\alpha$ Persei 
cluster. Columns as in Table 5. Cluster numbers are from Heckmann 
et al. (1956). Nonmember stars are identified with an asterisk in the Ref.
column.

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
 Star & HD/BD & $V$ &  $b-y$   &$m_{1}$  & $c_{1}$  &$\beta$   
&$\sigma_{V}$  & $\sigma_{b-y}$ &$\sigma_{m_{1}}$ & $\sigma_{c_{1}}$ 
&$\beta$  & N & Ref.  \\
\hline
& & & & & & & & & & & & & \\
247 & 20017  &   7.879 &   0.264 &  -0.022 &   0.646 &   2.616 &   0.002 &
       0.001 &   0.002 &   0.002 &   0.004 & 2 & 1,*\\
602 & +49$^{\circ}$ 916 &   9.594 &   0.187 &  -0.015 &   0.486 &   2.577 &  
&            &         &         &         & 1 & 2,* \\
955 & 21641  &   6.760 &   0.007 &   0.121 &   0.759 &   2.759 &         &
             &         &         &         & 1 & 3 \\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

1.- Wakerling (1970) \\
2.- Bidelman (1976) \\
3.- Merrill \& Burwell (1949) \\
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{\bf Table 9.} Photometric data for Be stars in the Orion OB1 
association. Columns as in Table 5. Cluster numbers are from Warren and 
Hesser (1977).

\begin{tabular}{rrrrrrrrr}
\hline
Star & HD/BD  & $V$ &  $b-y$ &  $m_{1}$  & $c_{1}$ & $\beta$ & N & Ref.\\
\hline
  & & & & & & & & \\
 20 & 34959 &    6.557 &   -0.023 &    0.074 &    0.579 &    2.605 & 1 & 1\\
 36 & 35407 &    6.305 &   -0.053 &    0.088 &    0.332 &    2.679 & 1 & 2\\
 38 & 35439 &    4.951 &   -0.074 &    0.065 &    0.050 &    2.527 & 1 & 3\\
 42 & 35502 &    7.339 &    0.002 &    0.109 &    0.336 &    2.708 & 1 & 1\\
266 & 36960 &    4.766 &   -0.106 &    0.068 &   -0.072 &    2.599 & 1 & 4\\
296 & 37041 &    5.064 &    0.017 &    0.017 &   -0.092 &    2.577 & 1 & 5\\
421 & 37490 &    4.506 &   -0.006 &    0.052 &    0.088 &    2.519 & 1 & 4\\
466 & 294304&   10.009 &    0.235 &    0.021 &    0.644 &    2.727 & 1 & 6\\
469 & 37806 &    7.901 &    0.036 &    0.105 &    0.778 &    2.710 & 1 & 6\\
523 & 39557 &    9.066 &    0.327 &    0.004 &    0.720 &    2.681 & 1 & 3\\
  & & & & & & & & \\
\hline
\end{tabular}

\begin{tabular}{ll}
 & \\
1.- Bidelman (1976)  & 4.- Morgan {\em et al.} (1955) \\
2.- Irvine (1975)    & 5.- Lesh (1968) \\
3.- Wakerling (1970) & 6.- Bartkus (1964) \\
\end{tabular}

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{\bf Table 10.} Photometric data for Be stars in NGC 2323. Columns as 
in Table 5. Cluster numbers are from Cuffey (1941).

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
Star & HD & $V$& $b-y$  & $m_{1}$ & $c_{1}$ &$\beta$ & $\sigma_{V}$   &
 $\sigma_{b-y}$& $\sigma_{m_{1}}$ & $\sigma_{c_{1}}$&$\sigma_{\beta}$ & 
N & Ref. \\
\hline
 & & & & & & & & & & & & & \\
 142 &--8$^{\circ}$ 1691 &  10.380 &   0.130 &   0.060 &   0.874 &   2.710 &   
0.015 &  0.007 &   0.001 &   0.009 &   0.009 & 2 & 1\\
 157 & 52922 &   9.294 &   0.131 &   0.056 &   0.665 &   2.658 &   0.001 &
       0.005 &   0.010 &   0.007 &   0.013 & 2 & 1\\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

1.- MacConnell (1961) \\
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{\bf Table 11.} Photometric data for Be stars in NGC 2422. Columns as 
in Table 5. Cluster numbers are from van Schewick (1966).

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
 Star & HD & $V$ & $b-y$ & $m_{1}$ & $c_{1}$  & $\beta$ & $\sigma_{V}$    &
    $\sigma_{b-y}$ & $\sigma_{m_{1}}$ & $\sigma_{c_{1}}$& 
$\sigma_{\beta}$&N & Ref. \\
\hline
 & & & & & & & & & & & & & \\
 42 & 60856 &   7.947 &   0.001 &   0.100 &   0.600 &   2.686 &   0.020 &
       0.002 &   0.006 &   0.010 &   0.001 &3 & 1\\
 45 & 60855 &   5.628 &   0.047 &   0.023 &   0.049 &   2.482 &   0.001 &
       0.002 &   0.006 &   0.004 &   0.002 &2 & 2\\
125 & 61224 &   6.534 &   0.039 &   0.068 &   0.767 &   2.647 &   0.023 &
       0.002 &   0.010 &   0.018 &   0.009 &3 & 2\\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

1.- Dworetski (1976) \\
2.- Wakerling (1970) \\
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{\bf Table 12.} Photometric data for Be stars in NGC 6611. Columns as 
in Table 5. Cluster numbers are from Walker (1961).

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
 Star & HD/BD  & $V$  &  $b-y$  & $m_{1}$ & $c_{1}$  & $\beta$  & 
$\sigma_{V}$&  $\sigma_{b-y}$ & $\sigma_{m_{1}}$ & $\sigma_{c_{1}}$ & 
$\sigma_{\beta}$& N & Ref.\\
\hline
 & & & & & & & & & & & & & \\
 205 & 168076  &   8.215 &   0.393 &  -0.077 &  -0.113 &   2.597 &   0.013 &
       0.006 &   0.009 &   0.005 &   0.009 & 4 & 1\\
 280 & -13$^{\circ}$ 4928  & 9.934 &   0.398 &  -0.087 &  -0.026 &   2.630 &  
&   &         &         &         & 1 & 2 \\
 503 & -13$^{\circ}$ 4936  & 9.626 &   0.500 &  -0.157 &  -0.146 &   2.518 &  
&   &         &         &         & 1 & 3 \\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

1.- Walker (1961) \\
2.- Hiltner (1956) \\
3.- Merrill \& Burwell (1949) \\
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{\bf Table 13.} Photometric data for Be stars in NGC 7654. Columns as 
in Table 5. Cluster numbers are from Lundby (1946).

\begin{tabular}{rrrrrrrrr}
\hline
  Star& BD   & $V$  &  $b-y$   & $m_{1}$  & $c_{1}$  & $\beta$  & N & 
Ref. \\
\hline
 & & & & & & & & \\
    778 &  &  11.834 &   0.456 &  -0.114 &   0.706 &   2.588 &1 & 1\\
    782 & +60$^{\circ}$ 2532d &  10.568 &   0.412 &  -0.034 &   0.606 &   
2.679 &1 & 2\\
    928 &  &  11.739 &   0.310 &   0.050 &   0.746 &   2.754 &1 & 2\\
    930 &  &  11.553 &   0.409 &  -0.059 &   0.581 &   2.684 &1 & 1\\
    989 &  &  11.858 &   0.430 &  -0.043 &   0.523 &   2.622 &1 & 1\\
 & & & & & & & & \\
\hline
\end{tabular}

1.- Bond (1973) \\
2.- Schild \& Romanishin (1976) \\
\rule{113mm}{0.1mm}
\clearpage

\thispagestyle{empty}
{\bf Table 14.} Photometric data for 
Be stars in the region of the Cepheus OB3 association. Columns as in Table 5. 
Nonmember stars are identified 
with an asterisk in the Ref. column. Association numbers are from Blaauw {\em 
et al.} (1959)

\begin{tabular}{rrrrrrrrrrrrrr}
\hline
 Star & HD/BD & $V$  & $b-y$   & $m_{1}$  & $c_{1}$ & $\beta$ & 
$\sigma_{V}$ & $\sigma_{b-y}$ & $\sigma_{m_{1}}$ & $\sigma_{c_{1}}$ & 
$\sigma_{\beta}$& N & Ref. \\ 
\hline
 & & & & & & & & & & & & & \\
 6 & +61$^{\circ}$ 2353 &   9.299 &   0.402 &   0.004 &   0.949 &   2.816 & 
0.062 &  0.118 &   0.106 &   0.458 &   0.101 &4 & 1,*\\
 9 & +61$^{\circ}$ 2355 &   9.617 &   0.302 &  -0.012 &   0.613 &   2.710 &   
0.004 &  0.004 &   0.007 &   0.030 &   0.019 &3 & 1,*\\
40 & 217061             &   8.768 &   0.535 &  -0.090 &   0.098 &   2.639 &
0.016 &  0.003 &   0.010 &   0.018 &   0.015 &3 & 2\\
51 & +61$^{\circ}$ 2380 &   9.145 &   0.154 &   0.077 &   0.966 &   2.845 &   
0.013 &  0.002 &   0.006 &   0.051 &   0.004 &3 & 1,*\\
64 & +61$^{\circ}$ 2382 &   9.571 &   0.236 &   0.067 &   1.185 &   2.846 &   
0.018 &  0.003 &   0.009 &   0.038 &   0.018 &3 & 1,*\\
65 & +62$^{\circ}$ 2158 &  10.108 &   0.203 &   0.050 &   0.934 &   2.838 &   
0.004 &  0.011 &   0.017 &   0.017 &   0.010 &3 & 1,*\\
80 & +61$^{\circ}$ 2396 &   9.568 &   0.135 &   0.121 &   0.992 &   2.849 &   
0.007 &  0.003 &   0.003 &   0.012 &   0.017 &2 & 1,*\\
 & & & & & & & & & & & & & \\
\hline
\end{tabular}

1.- Blaauw {\em et al.} (1959) \\
2.- Wakerling (1970) \\
\rule{173mm}{0.1mm}
\clearpage

\thispagestyle{empty}
{\bf Table 15.} Photometric data for B stars not classified as Be, observed 
in the open clusters and associations.
\small

\begin{tabular}{lrrrrrrrrrrrrrr}
\hline
Cluster & Star & HD/BD  & $V$ & $b-y$  & $m_{1}$ & $c_{1}$  & $\beta$ & 
$\sigma_{V}$ & $\sigma_{b-y}$& $\sigma_{m_{1}}$& $\sigma_{c_{1}}$& 
$\sigma_{\beta}$ &N & Notes \\
\hline
 & & & & & & & & & & & & & & \\
NGC 663 &  44 & +60$^{\circ}$ 339 & 8.490 &   0.543 &  -0.151 &   0.343 &   
2.593 & 0.013 & 0.004 &   0.006 &   0.008 &   0.006 & 5 & \\
        &  86 & +60$^{\circ}$ 331 & 8.980 &   0.678 &  -0.187 &   0.580 &   
2.612 & 0.020 & 0.004 &   0.005 &   0.010 &   0.005 & 5 & \\
        & 147 & +60$^{\circ}$ 347 & 9.538 &   0.640 &  -0.153 &   0.856 &   
2.656 &       &       &         &         &         & 1 & \\
 & & & & & & & & & & & & & & \\
h \& $\chi$ Per&  245 & +56$^{\circ}$ 481 &  9.891 &    0.220 &   -0.058 &    
0.014 & 2.616 & 0.009 &    0.015 &    0.021 &    0.023 &    0.005 & 2 & 2\\
               &  843 & +56$^{\circ}$ 510 &  9.339 &    0.281 &   -0.054 &    
0.149 & 2.615 & 0.006 &    0.007 &    0.009 &    0.012 &    0.017 & 11& 1\\
               &  864 & +56$^{\circ}$ 513 &  9.968 &    0.297 &   -0.052 &    
0.190 & 2.619 & 0.009 &    0.009 &    0.013 &    0.039 &    0.019 & 3 & \\
               &  936 & +56$^{\circ}$ 517 & 10.420 &    0.289 &   -0.059 &    
0.175 & 2.622 & 0.023 &    0.013 &    0.032 &    0.060 &    0.012 & 3 & \\
               &  978 & +56$^{\circ}$ 518 & 10.680 &    0.313 &   -0.038 &    
0.163 & 2.631 & 0.012 &    0.012 &    0.017 &    0.025 &    0.010 & 3 & \\
               & 1004 &                   & 10.885 &    0.318 &   -0.045 &    
0.182 & 2.644 & 0.033 &    0.008 &    0.022 &    0.041 &    0.025 & 3 & \\
               & 2139 &                   & 11.367 &    0.278 &   -0.048 &    
0.251 & 2.632 & 0.008 &    0.007 &    0.000 &    0.025 &    0.005 & 2 & \\
               & 2172 &  14434            &  8.497 &    0.191 &   -0.023 &   
-0.088& 2.576 & 0.006 &    0.006 &    0.009 &    0.012 &    0.008 & 23 & 1,2\\
               & 2196 &                   & 11.581 &    0.310 &   -0.069 &    
0.237 & 2.675 & 0.003 &    0.006 &    0.006 &    0.020 &    0.040 & 2 & \\
               & 2235 & +56$^{\circ}$ 571 &  9.369 &    0.316 &   -0.092 &    
0.143 & 2.602 & 0.037 &    0.023 &    0.035 &    0.022 &    0.011 & 3 & \\
               & 2251 &                   & 11.579 &    0.305 &   -0.051 &    
0.360 & 2.699 & 0.013 &    0.021 &    0.028 &    0.024 &    0.004 & 3 & \\
               & 2311 & +56$^{\circ}$ 576 &  9.388 &    0.292 &   -0.073 &    
0.153 & 2.630 & 0.004 &    0.003 &    0.001 &    0.001 &    0.005 & 2 & \\
               & 2361 & 14476             &  8.753 &    0.359 &   -0.103 &    
0.109 & 2.598 & 0.010 &    0.011 &    0.012 &    0.011 &    0.008 & 21 & 1\\
               & 2488 & +56$^{\circ}$ 586 &  9.938 &    0.274 &   -0.062 &    
0.093 & 2.612 & 0.035 &    0.003 &    0.021 &    0.016 &    0.008 & 3 & \\
 & & & & & & & & & & & & & & \\
$\alpha$ Per & 694 & 21092 &   8.498 &   0.108 &   0.199 &   0.943 &   
2.891 & 0.005 &  0.003 &   0.004 &   0.004 &   0.010 & 3 & 1 \\
             & 756 & 21239 &   7.949 &   0.063 &   0.184 &   0.999 &   
2.911 &  0.008 & 0.004 &   0.006 &   0.002 &   0.012 & 3 & 1 \\
             & 831 & 21398 &   7.372 &   0.018 &   0.132 &   0.837 &   
2.845 &  0.010 & 0.003 &   0.007 &   0.006 &   0.004 & 4 & 1 \\
 & & & & & & & & & & & & & & \\
Pleiades & 447 & 23288 &   5.456 &   0.001 &   0.101 &   0.634 &   
2.747 &   0.008 & 0.006 &   0.008 &   0.017 &   0.003 &8 & 1\\
         & 541 & 23324 &   5.659 &  -0.018 &   0.099 &   0.633 &   
2.745 &   0.004 & 0.002 &   0.005 &   0.010 &   0.004 &8 & 1\\
         & 563 & 23338 &   4.300 &  -0.034 &   0.095 &   0.564 &   
2.700 &    &  &         &         &         &1 &  \\
         & 785 & 23408 &   3.888 &  -0.011 &   0.092 &   0.600 &   
2.675 &    &  &         &         &         &1 & \\
         & 817 & 23432 &   5.775 &  -0.005 &   0.124 &   0.762 &   
2.786 &    &  &         &         &         &1 & \\
         &1823 & 23753 &   5.456 &  -0.014 &   0.094 &   0.726 &   
2.733 &    &  &         &         &         &1 & \\
         &2168 & 23850 &   3.610 &  -0.030 &   0.094 &   0.693 &   
2.694 &    &  &         &         &         &1 & \\
 & & & & & & & & & & & & & & \\
Ori OB1& 159 & 36591 &   5.326 &   -0.072 &    0.067 &    0.003 &    
2.617 & 0.001 & 0.001 & 0.003 & 0.001 & 0.004 & 2 & 1 \\
         & 482 & 37958 &   6.665 &   -0.022 &    0.128 &    0.915 &    
2.781 &       &       &       &       &       & 1 & \\
         & 489 & 38098 &   6.726 &    0.003 &    0.094 &    0.858 &    
2.691 &       &       &       &       &       & 1 & \\
 & & & & & & & & & & & & & & \\
NGC 2323&  1 & 52980 &   8.376 &   0.171 &   0.037 &   0.927 &   
2.727 & 0.026 &  0.004 &   0.005 &   0.002 &   0.002 & 2 & \\
 &  2 & --8$^{\circ}$ 1703 & 9.446 &   0.198 &   0.003 &   0.692 &   
2.724 & 0.161 &  0.039 &   0.027 &   0.060 &   0.021 & 2 & \\
 &  3        & 52965 &   9.161 &   0.112 &   0.047 &   0.564 &   
2.693 & 0.060 &  0.020 &   0.002 &   0.003 &   0.007 & 2 & 3\\
 & 51 & --8$^{\circ}$ 1708 & 9.946 &   0.137 &   0.050 &   0.544 &   
2.671 & 0.012 &  0.006 &   0.003 &   0.018 &   0.022 & 2 & \\
 & & & & & & & & & & & & & & \\
NGC 2422& 65 & 60940 &  8.703 &   0.027 &   0.092 &   0.775 &   2.809 &   
0.001 & 0.003 &   0.007 &   0.007 &   0.008 &2 & \\
 &   68       & 60942 &  9.212 &   0.037 &   0.137 &   0.854 &   2.827 &       
 
      &       &         &         &         &1 & \\
& 70 & -14$^{\circ}$ 2015 &   9.432 &   0.030 &   0.131 &   0.904 &   2.857 & 
0.001 & 0.006 &   0.012 &   0.006 &   0.001 &2 & \\
 &   71       & 60969 &  7.034 &  -0.002 &   0.083 &   0.502 &   2.687 &   
0.018 & 0.001 &   0.003 &   0.009 &   0.004 &4 & \\
 &   73       & 60995 &  8.643 &   0.020 &   0.103 &   0.787 &   2.755 &       
 
      &       &         &         &         &1 & \\
 &   78       & 60996 &  8.781 &   0.016 &   0.118 &   0.774 &   2.804 &       
      &       &         &         &         &1 & \\
& 79 & -14$^{\circ}$ 2022 &   7.775 &   0.008 &   0.097 &   0.537 &   2.726 &  
 
0.014 & 0.003 &   0.003 &   0.010 &   0.005 &4 & \\
&    83       & 61017 &   6.682 &   0.014 &   0.079 &   0.644 &   2.689 &   
0.001 & 0.000 &   0.003 &   0.012 &   0.001 &2 & \\
 & & & & & & & & & & & & & & \\
NGC 7654 
  &  735 &  &  10.820 &   0.457 &  -0.067 &   0.596 &   2.685 &&&&&&1 & \\
  &  852 &  &  14.071 &   0.353 &   0.112 &   1.008 &   2.784 &&&&&&1 & \\
  &  870 &  &  13.523 &   0.398 &   0.029 &   0.926 &   2.938 &&&&&&1 & \\
  &  884 &  &  12.174 &   0.372 &  -0.040 &   0.531 &   2.738 &&&&&&1 & \\
  &  984 &  &  13.231 &   0.480 &  -0.083 &   0.887 &   2.754 &&&&&&1 & \\
 & & & & & & & & & & & & & & \\
\hline

\end{tabular}
\pagebreak
\thispagestyle{empty}
\normalsize
{\bf Table 15.} (Continued)
\small

\begin{tabular}{lrrrrrrrrrrrrrr}
\hline
Cluster & Star & HD/BD  & $V$ & $b-y$  & $m_{1}$ & $c_{1}$  & $\beta$ & 
$\sigma_{V}$ & $\sigma_{b-y}$& $\sigma_{m_{1}}$& $\sigma_{c_{1}}$& 
$\sigma_{\beta}$ &N & Notes \\
\hline
 & & & & & & & & & & & & & & \\
Cep OB3
& 2 & +61$^{\circ}$ 2350 &   9.204 &   0.602 &  -0.172 &   0.150 &   2.633 & 
0.012 &  0.004 &   0.009 &   0.005 &   0.007 &5 &1\\
&10 & 216532             &   8.020 &   0.478 &  -0.143 &   0.018 &   2.617 & 
0.014 &  0.003 &   0.005 &   0.014 &   0.006 &3 &1\\
&15 & 216629             &   9.294 &   0.582 &  -0.111 &   0.160 &   2.591 & 
 0.059 &  0.011 &   0.008 &   0.011 &   0.010 &5 & 4\\
&9 &                    &  10.351 &   0.329 &   0.007 &   0.434 &   2.685 & 
&              &         &         &         &1 &\\
&4 & +61$^{\circ}$ 2366 &   9.705 &   0.592 &  -0.156 &   0.131 &   2.631 & 
0.012 &  0.008 &   0.015 &   0.011 &   0.030 &2 &\\
&39 & 217035             &   7.758 &   0.414 &  -0.117 &   0.007 &   2.616 & 
0.012 &  0.001 &   0.005 &   0.014 &   0.006 &5 &1\\
&41 & 217086             &   7.662 &   0.530 &  -0.158 &  -0.001 &   2.607 & 
0.008 &  0.003 &   0.003 &   0.011 &   0.003 &4 &1\\
&50 & +62$^{\circ}$ 2150 &   9.764 &   0.376 &  -0.040 &   0.369 &   2.709 & 
0.005 &  0.007 &   0.008 &   0.024 &   0.009 &2 &\\
&56 & +62$^{\circ}$ 2154 &   9.300 &   0.423 &  -0.077 &   0.134 &   2.620 & 
0.009 &  0.007 &   0.024 &   0.014 &   0.014 &2 &\\
 & & & & & & & & & & & & & & \\
\hline
\end{tabular}

\normalsize
1.- Used as standard \\
2.- Nonmember of the cluster or association \\
3.- Chemically peculiar star (Ap or Am, Renson 1988) \\
4.- Variable star IL Cephei. Herbig Ae/Be star. \\
\rule{185mm}{0.1mm}
\end{document}
