Table 1: Millimeter flux densities, sizes, spectral indices and masses.
\begin{displaymath}\begin{tabular}{l c c c c c } %
\hline\hline
\\
\multicolum...
...& 0.8 & $-0.1$ & $\le$0.0 &
$\le$0.0 \\
\hline
\end{tabular}\end{displaymath}
a Masses have to be scaled up by a factor of $\sim$6 for a dust temperature of 20 K.

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