\begin{table}%t4 
\caption {\label{propBe}Number ratios of Be to (B+Be) stars as a function of spectral 
type in SMC and Galaxy$^{1}$. }
%\centerline
 {
\begin{tabular}{llll}
\hline
\hline	
Spectral type      & SMC & SMC \% &  Galaxy  \\
                   & \%  & without NGC~330 &  \% \\
\hline	
O8-O9e	& 23.8	& 20.8 & 14.3 \\
B0e	& 35.2	& 26.3 & 7.6  \\  
all B0e & 36.1  &      & 12.7 \\
B1e     & 20.6  & 16.7 & 3.4  \\
all B1e & 27.0  &      & 7.7  \\
B2e     & 15.3  & 13.9 & 4.9  \\
all B2e & 19.9  &      & 7.8  \\
B3e     & 9.6   & 8.9  & 3.4  \\
all B3e & 14.0  &      & 6.8  \\
B4e     & 2.9   & 3.0  & 0.0  \\
all B4e & 7.6   &      & 0.0  \\
B5e     & 0.0   & 0.0  & 2.2  \\
all B5e & 1.8   &      & 9.2  \\
B6e     & 0.6   & 0.6  & 0.0  \\
all B6e & 1.2   &      & 0.0  \\
B7e     & 0.0   & 0.0  & 2.4  \\
all B7e & 0.0   &      & 7.2  \\
B8e     & 0.0   & 0.0  & 1.2  \\
all B8e & 0.0   &      & 9.3  \\
B9e     & 0.0   & 0.0  & 1.8  \\
all B9e & 0.0   &      & 11.1 \\
A0e     & 2.5   & 2.5  & 0.9  \\
\hline	
\end{tabular}}
\par
\smallskip
$^1$ {\scriptsize For each range in spectral type, the
fractions of definite emission-line stars and the combination of
definite and candidate emission-line stars are listed.}
\end{table}