\begin{table}%T5
\caption{ The continuum flux at the peak wavelength of the IR
features included in this analysis. When the amorphous 10~micron
silicate band was present, the PAH features are superimposed on the
band. In this case (flagged by $^\ast$), the silicate feature is
regarded as being part of the underlying 
continuum of the PAH features. Hence the indicated continuum flux
of the PAH band is the flux of the silicate feature at the central
wavelength of that PAH band.
 \label{CF}}	
%\centering
\par
\begin{tabular}{cccccccccc}
 \hline \hline
 \multicolumn{10}{c}{\bf CF at the peak wavelength of the IR features}\\ \hline
 \multicolumn{1}{c}{Object} &
 \multicolumn{1}{c}{Group} &
 \multicolumn{1}{c}{PAH 3.3} & 
 \multicolumn{1}{c}{NAN 3.4} & 
 \multicolumn{1}{c}{NAN 3.5} &
 \multicolumn{1}{c}{PAH 6.2} &
 \multicolumn{1}{c}{PAH 7.7} &
 \multicolumn{1}{c}{PAH 8.6} &
 \multicolumn{1}{c}{COMP 11} &
 \multicolumn{1}{c}{Si 9.7} \\ 
                 &    &  [Jy]  &  [Jy]  &  [Jy] &  [Jy] &  [Jy]      &  [Jy] &  [Jy] &  [Jy] \\
\hline
\object{V376 Cas}         & I  &   5.5  &   6.0  &   6.3 &  10.0 &  11.3$^\ast$&  17.1$^\ast$&  23.2$^\ast$&  13.7 \\
\object{Elias 3-1}        & I  &   3.1  &   3.3  &   3.5 &   4.0 &   8.0$^\ast$&  12.4$^\ast$&  32.7$^\ast$&  19.1 \\
\object{AB Aur}           & I  &  13.1  &  13.1  &  13.0 &   9.1 &  10.0$^\ast$&  15.1$^\ast$&  24.8$^\ast$&  12.8 \\
\object{HD~34282}         & I  &   0.7  &   0.8  &   0.7 &   1.0 &   0.9      &   0.8      &   0.8      &   0.7 \\
\object{HD~34700}         & I  &   0.5  &   0.5  &   0.3 &   0.4 &   0.7      &   0.7      &   0.8      &   0.7 \\
\object{HD~97048}         & I  &   2.0  &   2.0  &   2.0 &   1.1 &   3.2      &   4.0      &   6.4      &   4.7 \\
\object{HD~100453}        & I  &   4.8  &   4.9  &   4.9 &   3.7 &   4.4      &   4.2      &   6.3      &   4.7 \\
\object{HD~100546}        & I  &   6.0  &   5.7  &   5.7 &   7.0 &  17.3$^\ast$&  28.8$^\ast$&  62.5$^\ast$&  28.4 \\
\object{HD~135344}        & I  &   3.4  &   3.4  &   3.4 &   2.1 &   1.7      &   1.4      &   1.0      &   1.1 \\
\object{HD~139614}        & I  &   1.4  &   1.3  &   1.3 &   1.0 &   1.4      &   1.5      &   2.6      &   2.4 \\
\object{HD~142527}        & I  &   6.4  &   6.4  &   6.4 &   7.0 &   7.7$^\ast$&  10.7$^\ast$&  11.9$^\ast$&   7.1 \\
\object{CD$-$42$^\circ$11721}& I& 23.6  &  25.0  &  25.7 &  41.4 &  44.3      &  43.7      &  45.9      &  39.5 \\
\object{HD~169142}        & I  &   1.8  &   1.7  &   1.7 &   1.7 &   1.6      &   1.6      &   2.0      &   1.6 \\
\object{T CrA}            & I  &   2.2  &   2.2  &   2.3 &   3.0 &   3.3$^\ast$&   4.4$^\ast$&   8.3$^\ast$&   5.9 \\
\object{HD~179218}        & I  &   3.4  &   3.4  &   3.5 &   5.5 &   9.3$^\ast$&  14.2$^\ast$&  18.3$^\ast$&  10.5 \\
\object{BD+40$^\circ$4124} & I? &  5.5  &   5.6  &   5.7 &   7.5 &   9.0      &   9.6      &   8.9      &   8.1 \\
\object{HD~200775}        & I  &  11.8  &  11.7  &  11.8 &   9.4 &   9.8$^\ast$&  11.4$^\ast$&   9.3$^\ast$&   8.2 \\
\object{MWC 1080}         & I  &  11.2  &  11.6  &  11.7 &  14.5 &  14.9      &  14.6      &  16.2      &  13.6 \\
\hline		 			 	 	 	 	 	 		       	       	
\object{VX Cas}           & II &   0.4  &   0.4  &   0.4 &   0.4 &   0.5$^\ast$&   0.8$^\ast$&   1.2$^\ast$&   0.7 \\
\object{HD~31648}         & II &   4.0  &   4.0  &   4.0 &   4.6 &   6.1$^\ast$&   8.7$^\ast$&  11.3$^\ast$&   6.1 \\
\object{UX Ori}           & II &   0.9  &   0.9  &   0.9 &   0.8 &   0.9$^\ast$&   2.0$^\ast$&   2.7$^\ast$&   1.5 \\
\object{HD~35187}         & II &   2.4  &   2.4  &   2.4 &   1.9 &   2.6      &   3.8      &   5.4      &   4.9 \\
\object{BF Ori}           & II &   0.4  &   0.4  &   0.4 &   0.5 &   0.6$^\ast$&   1.1$^\ast$&   1.4$^\ast$&   0.8 \\
\object{RR Tau}           & II &   0.9  &   0.9  &   0.9 &   0.9 &   1.1      &   1.2      &   1.6      &   1.3 \\
\object{HD~95881}         & II &   4.0  &   3.9  &   3.9 &   4.5 &   5.5      &   6.9      &   7.8      &   8.0 \\
\object{HD~104237}        & II &  10.8  &  10.8  &  10.8 &  10.8 &  10.6$^\ast$&  15.9$^\ast$&  22.4$^\ast$&   9.6 \\
\object{HD~141569}        & II &   0.7  &   0.7  &   0.6 &   0.4 &   0.5      &   0.5      &   0.5      &   0.5 \\
\object{HD~142666}        & II &   2.7  &   2.7  &   2.7 &   0.6 &   3.7$^\ast$&   5.5$^\ast$&   6.3$^\ast$&   2.6 \\
\object{HD~144432}        & II &   2.8  &   2.8  &   2.7 &   2.1 &   2.3$^\ast$&   4.8$^\ast$&   7.4$^\ast$&   4.1 \\
\object{HR 5999}          & II &  17.9  &  18.0  &  18.1 &  13.6 &  13.9$^\ast$&  15.0$^\ast$&  16.9$^\ast$&  14.7 \\
\object{Wra 15-1484}      & II &   6.6  &   7.1  &   7.4 &  14.4 &  17.3      &  18.4      &  21.0      &  19.8 \\
\object{HD~150193}        & II &   4.8  &   4.7  &   4.7 &   4.8 &   5.5$^\ast$&  13.3$^\ast$&  18.7$^\ast$&   8.8 \\
\object{AK Sco}           & II &   1.5  &   1.5  &   1.5 &   1.2 &   1.2$^\ast$&   1.9$^\ast$&   2.8$^\ast$&   2.0 \\
\object{HD~163296}        & II &   9.8  &   9.7  &   9.6 &   7.2 &   8.8$^\ast$&  14.0$^\ast$&  20.3$^\ast$&  12.2 \\
\object{VV Ser}           & II &   2.5  &   2.5  &   2.5 &   2.6 &   3.1$^\ast$&   3.8$^\ast$&   4.4$^\ast$&   3.4 \\
\object{R CrA}            & II?&  54.2  &  57.0  &  59.2 &  64.6 &  58.3$^\ast$&  79.8$^\ast$& 126.3$^\ast$&  86.1 \\
\object{WW Vul}           & II &   0.9  &   0.9  &   0.8 &   0.7 &   0.8$^\ast$&   1.5$^\ast$&   2.1$^\ast$&   1.3 \\
\object{LkH$\alpha$ 224}  & II?&   3.9  &   4.1  &   4.2 &   7.3 &   9.0      &  10.3      &  12.4      &  11.4 \\
\object{BD+46$^\circ$3471} & II &       &        &       &   0.6 &   0.9$^\ast$&   1.0$^\ast$&   1.6$^\ast$&   1.0 \\	       
\object{SV Cep}           & II &   0.6  &   0.7	&   0.7	&   0.8 &   1.1$^\ast$&   2.9$^\ast$&   4.6$^\ast$&   2.7 \\       
\hline		 		      	 	 	 	 	 	
\object{Z CMa}            & III&  40.1  &  43.3  &  45.2 &  86.9 & 101.7      &  84.3      & 101.9      & 114.7 \\
\object{IRAS 12496-7650}	 & III&   7.9  &   9.1  &   9.7 &  17.7 &  21.8      &  21.8      &  33.3      &  30.2 \\
\object{MWC 297}          & III&  65.8  &  68.3  &  71.5 & 104.6 & 118.9      & 123.7      & 119.7      & 123.3 \\
\object{LkH$\alpha$ 225}  & III&   1.3  &   1.5  &   1.7 &  12.6 &  24.5      &  23.8      &  26.2      &  36.8 \\
\object{PV Cep}           & III&   1.9  &   2.2  &   2.4 &   7.4 &   9.6      &   8.5      &  10.6      &  12.8 \\
\object{V645 Cyg}         & III&   8.3  &   9.6  &  10.7 &  45.2 &  65.7      &  65.4      &  87.5      &  91.0 \\
\hline
\end{tabular}		    
\end{table}