\begin{table} %TA.4
%\centering
\par
\caption{IRAS photometry points at $12$, $25$, $60$ and $850
~\mu$m. Note however that in some cases the $100~\mu$m is an upper
limit (L); these observations are probably contaminated by
interstellar cirrus clouds. For RV~Tau the $100~\mu$m data point is
a lower limit (:).}
\begin{tabular}{l|llll}
\hline\hline
Name	&$F_{12}$(Jy)	&$F_{25}$(Jy)	&$F_{60}$(Jy)	&$F_{100}$(Jy)\\
\hline
TW~Cam	&8.25		&5.60		&1.84		&1.79L\\
\par
RV~Tau	&22.52		&18.05		&6.50		&2.44:\\
\par
SU~Gem	&7.91		&5.68		&2.19		&11.99L\\
\par
UY~CMa	&3.49		&2.46		&0.57		&1.00L\\
\par
U~Mon	&124.30		&88.43		&26.59		&9.54\\	
\par
AC~Her	&41.43		&65.33		&21.37		&8.04\\
\par
R~Sct	&20.83		&9.26		&8.20		&140.30L\\
\hline
\end{tabular}
\label{DATA:IRAS}
\end{table}