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{\Large {\bf Table 7a} : comparison of 400 $\mu$m fluxes and model
predictions (1. Jones \& Merrill (1976), 2. Table 8)\\}
\begin{center}
\begin{small}
\begin{tabular}{ccccccccccc}
\hline
Grain & Name & Phase & Observation & n$_{H}$=0 & n$_{H}$=0 & n$_{H}$=1 & n$_{H}$=1 & 
n$_{H}$=10 & n$_{H}$=10\\
model & &  & $\phi$ = 37" & F$_{\rm tot}$ & $\phi$ = 37" & F$_{\rm tot}$ & 
$\phi$ = 37" & F$_{\rm tot}$ & $\phi$ = 37" \\
\hline
& & & & & & & & \\
1& NML Tau     & 0.92 & $<$4 &  2.0 & 0.67 & 18   & 0.68 & 172  & 0.7 \\
1& OH 26.5+0.6 & 0.36 &      & 2.36 & 0.55 & 2.38 & 0.55 & 3.61 & 0.56 \\
1& IRC --10529 & 0.78 & $<$7 & 0.91 & 0.22 & 1.2  & 0.23 & 6.87 & 0.23 \\
\hline
& & & & & & & \\
2& NML Tau     & 0.92 & $<$4 & 4.14 & 0.97 & 30   & 0.97 & 284  & 1.01 \\
2& OH 26.5+0.6 & 0.36 &      & 5.3  & 1.5  & 5.4  & 1.5  & 7.3  & 1.5 \\
2& IRC --10529 & 0.78 & $<$7 & 2.05 & 0.48 & 2.42 & 0.49 & 11.6 & 0.50\\
\hline
\end{tabular}
\end{small}
\end{center}
\vspace*{0.7cm}

{\Large {\bf Table 7b} : comparison of 800 $\mu$m fluxes and model
predictions (1. Jones \& Merrill (1976), 2. Table 8)\\}
\begin{center}
\begin{small}
\begin{tabular}{cccccccccc}
\hline
Grain & Name & Phase & Obs. &  n$_{H}$=0 & n$_{H}$=0 & n$_{H}$=1 & n$_{H}$=1 & 
n$_{H}$=10 & n$_{H}$=10\\
model & & & $\phi$ = 16" & F$_{\rm tot}$ & $\phi$ = 16" & F$_{\rm tot}$ & 
$\phi$ = 16" & F$_{\rm tot}$ & $\phi$ = 16"\\
\hline
& & & & & & & & \\
1 & NML Tau     & 0.92 & 0.245 & 0.279 & 0.14 & 2.0  & 0.14 & 19   & 0.14 \\
1 & OH 26.5+0.6 & 0.36 & 0.1   & 0.24  & 0.04 & 0.24 & 0.04 & 0.38 & 0.04 \\
1 & IRC --10529 & 0.78 &       & 0.1   & 0.03 & 0.13 & 0.03 & 0.78 & 0.03\\
\hline
& & & & & & & & \\ 
2& NML Tau     & 0.92 & 0.245 & 0.49 & 0.17  & 3.6  & 0.17  & 342  & 0.17 \\
2& OH 26.5+0.6 & 0.36 & 0.1   & 0.56 & 0.085 & 0.57 & 0.085 & 0.86 & 0.086\\
2& IRC --10529 & 0.78 &       & 0.22 & 0.042 & 0.27 & 0.043 & 1.45 & 0.044\\
\hline 

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

\vspace*{0.7cm}
{\Large {\bf Table 7c} : comparison of 1100 $\mu$m fluxes and model
predictions (1. Jones \& Merrill (1976), 2. Table 8)\\}

\begin{center}
\begin{small}
\begin{tabular}{ccccccccccc}
\hline
Grain & Name & Phase & Obs. & n$_{H}$=0 & n$_{H}$=0 & n$_{H}$=1 & n$_{H}$=1 &
n$_{H}$=10 & n$_{H}$=10\\
model & & & $\phi$ = 19" & F$_{\rm tot}$ & $\phi$ = 19" & F$_{\rm tot}$ & 
$\phi$ = 19" & F$_{\rm tot}$ & $\phi$ = 19"\\
\hline
& & & & & & & & \\
1 & NML Tau     & 0.92 & 82 & 118  & 75   & 716  & 76   & 6400 & 76 \\
1 & OH 26.5+0.6 & 0.36 & 48 & 79.5 & 16.4 & 80.3 & 16.6 & 130  & 16.7  \\
1 & IRC --10529 & 0.78 &    & 37.4 & 14.8 & 48.9 & 15.2 & 256  & 15.2\\
\hline
& & & & & & & & \\
2& NML Tau     & 0.92 & 82 & 187 & 85 & 1135 & 86 & 11210 & 86 \\
2& OH 26.5+0.6 & 0.36 & 48 & 184 & 31 & 186  & 31 &   284 & 32\\
2& IRC --10529 & 0.78 &    & 76  & 19 & 93   & 20 &   490 & 20\\
\hline

\end{tabular}
\end{small}
\end{center}
\vspace*{0.7cm}

{\Large {\bf Table 7d} : comparison of 1300 $\mu$m fluxes and model
predictions (1. Jones \& Merrill (1976), 2. Table 8)\\}

\begin{center}
\begin{small}
\begin{tabular}{cccccccccccccc}
\hline
Grain & Name  & Phase &Obs.& n$_{H}$=0&n$_{H}$=0&n$_{H}$=0&n$_{H}$=1&n$_{H}$=1&
n$_{H}$=1&n$_{H}$=10&n$_{H}$=10&n$_{H}$=10\\
model & &  & & F$_{\rm tot}$ & $\phi$=24" &$\phi$=11" & F$_{\rm tot}$ & $\phi$=24"&
$\phi$=11"& F$_{\rm tot}$ & $\phi$=24"&$\phi$=11"\\
\hline
& & & & & & & & &\\
1 & NML Tau     & 0.92 & 36.7$^{2}$ & 77   & 53   & 53  & 406  & 54   & 54  &
 3542 & 54 & 54\\
1 & OH 26.5+0.6 & 0.36 & 69$^{1}$   & 44.7 & 11.2 & 9.3 & 44.8 & 11.2 & 9.4 &
 72.3 & 11.2 & 9.5  \\
1 & IRC --10529 & 0.78 &            & 22.4 & 10   & 10  & 28.7 & 10   & 10  &
 142 & 10 & 10\\
\hline
& & & & & & & & \\
2& NML Tau     & 0.92 & 36.7$^{2}$ & 114 & 60 & 59 & 676 & 60 & 59  & 6120 & 
60 & 59  \\
2& OH 26.5+0.6 & 0.36 & 69$^{1}$   & 102 & 20 & 15 & 102 & 20 & 15  & 158  & 
20 & 15  \\
2& IRC --10529 & 0.78 &            & 43  & 13 & 12 &  53 & 13 & 12  & 271  & 
13 & 12  \\
\hline

\end{tabular}
\end{small}
\end{center}
$^{1}$ $\phi$=24",  $^{2}$  $\phi$=11"\\


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

\end{document}


