\begin{table}%t3
\caption{\label{cont_tab}Peak position, angular and linear diameter, integrated flux density, mass, H$_2$ volume 
and column density of the millimeter condensations~C1 (resolved into C1-a and C1-b in the 284~GHz image) and 
C2. The masses are computed for $\beta = 2$, and assuming $T$ = 30~K. The H$_2$~volume and
column densities are calculated assuming a spherical source with diameter equal to the deconvolved
3$\sigma$ level.}
%\centerline
 {
\begin{tabular}{ccccccccc}
\hline \hline
\multicolumn{9}{c}{$\nu = 96$~GHz} \\
Source & \multicolumn{2}{c}{Peak position} & \multicolumn{2}{c}{Diameter}  & $F_{\nu}$ & $M_{\rm cont}$ & $n_{\rm H_2}$  & $N({\rm H_2})$ \\[-3.2mm]\\
\cline{2-3} \cline{4-9} 
       & RA(J2000) & Dec(J2000)  & $\theta_{\rm s}$  & $D$  & &  &  & \\
       & $\rm 05^h37^m$ &   & (\asec)& (pc) & (mJy) & ($M_{\odot}$) & ($\times 10^6$ \cmc ) & ($\times 10^{23}$ \cmq )  \\
C1$^{\bf *}$ & 52$\fs$17 & +32$ \degr$00$^{\prime}$04$\farcs$5 & 9.08 & 0.08  &  11 & 27 & 2.1 &  5.2 \\
C2 & 52$\fs$91 & $+31\degr59^{\prime}58\farcs5$ & 6.35 & 0.06  &  6  & 15 & 2.8 &  5.2 \\
\hline
\multicolumn{9}{c}{$\nu = 225$~GHz} \\
Source & \multicolumn{2}{c}{Peak position}  & \multicolumn{2}{c}{Diameter}  & $F_{\nu}$ & $M_{\rm cont}$ & $n_{\rm H_2}$ &  $N({\rm H_2})$ \\[-3.2mm]\\
\cline{2-3} \cline{4-9} 
       & RA(J2000) & Dec(J2000)  & $\theta_{\rm s}$  & $D$  & & & & \\
       & $\rm 05^h37^m$ &   & (\asec)& (pc) & (mJy) & ($M_{\odot}$) & ($\times 10^6$ \cmc ) & ($\times 10^{23}$ \cmq )  \\
C1$^{\bf *}$ & 52$\fs$19 & +32$ \degr$00$^{\prime}$05 & 7.3 & 0.06  &  150 & 12 & 1.4 &  3.0 \\
C2 & 52$\fs$90 & +31$ \degr$59$^{\prime}$58$\farcs$5 & 5.3 & 0.05  &  60  & 4.7 & 1.2 &  2.0 \\
\hline
\multicolumn{9}{c}{$\nu = 284$~GHz} \\
Source & \multicolumn{2}{c}{Peak position}  & \multicolumn{2}{c}{Diameter}  & $F_{\nu}$ & $M_{\rm cont}$ & $n_{\rm H_2}$ &  $N({\rm H_2})$ \\[-3.2mm]\\
\cline{2-3} \cline{4-9} 
       & RA(J2000) & Dec(J2000)  & $\theta_{\rm s}$  & $D$  & & & & \\
       & $\rm 05^h37^m$ &   & (\asec)& (pc) & (mJy) & ($M_{\odot}$) & ($\times 10^6$ \cmc ) & ($\times 10^{23}$ \cmq )  \\
C1-b & 52$\fs$17 & +32$ \degr$00$^{\prime}$04 & 1.8 & 0.016  &  160 & 5.2;  0.6$^{\dagger}$ & 8.5;  1.0$^{\dagger}$ & 7.6; 0.9$^{\dagger}$  \\
C1-a & 52$\fs$27 & +32$ \degr$00$^{\prime}$06 & 2.1 & 0.018  &  115  & 3.6 & 6.6 &  5.7 \\
C2  & 52$\fs$90 & +31$ \degr$59$^{\prime}$58 & 1.5 & 0.013  &  90  & 2.9 & 10.9 &  7.4 \\
\hline
\end{tabular}}
\par
\medskip
$^{\bf *}$  C1-a + C1-b. \\
$^{\dagger}$  Computed from the CH$_3$CN temperature of 200 K.
\end{table}