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{\Large {\bf Table 6a} : comparison of 60 $\mu$m IRAS fluxes and model
predictions (1. Jones \& Merrill (1976), 2. Table 8)\\}
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\begin{center}
\begin{small}
\begin{tabular}{ccccccccccc}
\hline
Grain & Name & Phase & IRAS & n$_{H}$=0 & n$_{H}$=0 & n$_{H}$=1 & n$_{H}$=1 & 
n$_{H}$=10 & n$_{H}$=10\\
model &    & & & F$_{\rm tot}$ & $\phi$ = 3.15' & F$_{\rm tot}$ & $\phi$ = 3.15' & 
F$_{\rm tot}$& $\phi$ = 3.15'\\
\hline
& & & & & & & & \\
1& NML Tau     & 0.92 & 257.45 & 199 & 182 & 222 & 183 & 503 & 191 \\
1& OH 26.5+0.6 & 0.36 & 373.39 & 239 & 238 & 240 & 238 & 240 & 238\\
1& IRC --10529 & 0.78 & 168.37 & 95  & 93  &  96 &  94 & 100 &  94\\
\hline
& & & & & & & \\
2& NML Tau     & 0.92 & 257.45  & 299 & 285 & 300 & 285 & 402 & 288 \\
2& OH 26.5+0.6 & 0.36 & 373.39  & 338 & 338 & 339 & 339 & 339 & 339\\
2& IRC --10529 & 0.78 & 168.37  & 144 & 143 & 144 & 143 & 144 & 143\\
\hline
\end{tabular}
\end{small}
\end{center}
\vspace*{0.7cm}

{\Large {\bf Table 6b} : comparison of 100 $\mu$m IRAS fluxes and model
predictions (1. Jones \& Merrill (1976), 2. Table 8)\\}
\vspace*{0.5cm}
\begin{center}
\begin{small}
\begin{tabular}{ccccccccccc}
\hline
Grain & Name & Phase & IRAS & n$_{H}$=0 & n$_{H}$=0 & n$_{H}$=1 & n$_{H}$=1 & 
n$_{H}$=10 & n$_{H}$=10\\
model &   & & & F$_{\rm tot}$ & $\phi$ = 4.25' & F$_{\rm tot}$ & $\phi$ = 4.25' & 
F$_{\rm tot}$ & $\phi$ = 4.25'\\
\hline
& & & & & & & & \\
1 & NML Tau     & 0.92 & 95.16  & 47 & 35 & 112 & 36 & 788 & 49 \\
1 & OH 26.5+0.6 & 0.36 & $<$288 & 53 & 50 &  54 & 51 &  55 & 51 \\
1 & IRC --10529 & 0.78 & 58.93  & 21 & 19 &  22 & 19 &  39 & 20\\
\hline
& & & & & & & & \\ 
2& NML Tau     &  0.92 & 95.16  & 111 &  92 & 162 &  92 & 779 & 116 \\
2& OH 26.5+0.6 & 0.36  & $<$288 & 133 & 131 & 133 & 131 & 133 & 131\\
2& IRC --10529 & 0.78  & 58.93  & 54  &  51 &  54 &  51 &  65 & 53\\
\hline 

\end{tabular}
\end{small}
\end{center}
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{\Large {\bf Table 6c} : model predictions of fluxes at 200 $\mu$m 
(1. Jones \& Merrill (1976), 2. Table 8)\\}
\vspace*{0.5cm}
\begin{center}
\begin{small}
\begin{tabular}{ccccccccc}
\hline
Grain & Name & Phase & n$_{H}$=0 & n$_{H}$=0 & n$_{H}$=1 & n$_{H}$=1 & 
n$_{H}$=10 & n$_{H}$=10\\
model &      &  & F$_{\rm tot}$ & $\phi$ = 90" & F$_{\rm tot}$ & $\phi$ = 90" &
F$_{\rm tot}$ & $\phi$ = 90"\\
\hline
& & & & & & & \\
1 & NML Tau     & 0.92 & 12    & 4.4  & 83   & 4.5 & 770  & 52 \\
1 & OH 26.5+0.6 & 0.36 & 14.7  & 7.7  & 14.8 & 7.8 & 18.9 & 7.7 \\
1 & IRC --10529 & 0.78 & 5.76  & 2.48 & 8.87 & 2.5 & 29.7 & 2.64\\
\hline
& & & & & & &  \\ 
2 & NML Tau      & 0.92 & 26  & 9.6   & 116 & 9.6 & 1039 & 11 \\
2 & OH 26.5+0.6  & 0.36 & 32  & 21    & 32  &  21 & 37   & 21 \\
2 & IRC --10529  & 0.78 & 13  & 6.7   & 13  & 6.7 & 41   & 6.9\\
\hline
\end{tabular}
\end{small}
\end{center}

Note:\\
all fluxes are in Jy and the interstellar densities are expressed in H cm$^{-3}$

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