\begin{table}%t4
%\centering
\par
\caption{Input physical parameters for DUSTY and the adopted reddening values.}\label{t4}
\begin{tabular}{cccccccc} \hline\hline
IRAS & Dust & $E(B-V)$    & $E(B-V)$ & $T_{\rm eff}$ & Grain types$^{\dagger}$ & Optical depth & $T_{\rm d}$ \\
     & type & total       &  I.S.    & (K)     &                           & ($\tau$) at 0.55~$\mu$ & (K)  \\ 
\hline  
12584--4837$^{*}$ & warm$^{1}$ & 0.27 & 0.18 & 20~000 & amC-Hn & 0.26 & 775 \\
                 & warm$^{2}$ & 0.27 & 0.18 & 20~000 & amC-Hn & 0.29 & 700 \\
           & cold & 0.27 & 0.18 & 20~000 & Sil-DL \& SiC & 0.29 & 200 \\
13266--5551 & cold & 0.51 & 0.53 & 20~800 & grf-DL & 0.12 & 160 \\
14331--6435 & cold & 0.71 &  --  & 16~200 & Sil-Ow & 0.50 & 130 \\
16206--5956 & cold & 0.29 & 0.22 & 11~200 & grf-DL \& amC-Hn & 0.16 & 170 \\
17203--1534 & cold & 0.61 & 0.44 & 19~000 & Sil-Ow & 0.15 & 117 \\
17311--4924 & cold & 0.66 & 0.22 & 20~300 & grf-DL \& SiC-Pg & 0.22 & 250 \\
17423--1755 & warm & 0.86 & 0.67 & 20~000 & amC-Hn & 0.16 & 1500 \\
           & warm & 0.86 & 0.67 & 20~000 & amC-Hn & 0.32 & 1000 \\    
           & cold & 0.86 & 0.67 & 20~000 & SiC-Pg & 0.35 & 100 \\ 
17460--3114 & cold & 0.54 & --   & 35~000 & Sil-DL \& grf-DL & 0.0015 & 315 \\
18023--3409 & cold & 0.70 & 0.44 & 20~300 & grf-DL & 0.015 & 220 \\
18062+2410$^{*}$ & cold & 0.24 & 0.11 & 20~750 & Sil-Oc \& Sil-DL & 0.32 & 230 \\
18371--3159 & cold & 0.30 & 0.15 & 20~800 & grf-DL & 0.13 & 180 \\ 
18379--1707$^{*}$ & cold & 0.71 & --   & 19~000 & Sil-DL & 0.13 & 140 \\
19590--1249 & cold & 0.29 & 0.20 & 20~500 & Sil-Ow \& Sil-DL & 0.08 & 120 \\
22023+5249 & cold & 0.85 & --   & 18~500 & Sil-Oc \& Sil-DL & 0.29 & 120 \\
22495+5134 & cold & 0.52 & 0.36 & 35~000 & Sil-DL & 0.011 & 125 \\
\hline
\end{tabular}
$^{\dagger}$ The grain types used for modelling the SEDs are
"warm'' (Sil-Ow) and "cold'' (Sil-Oc) silicates from Ossenkopf et~al. (\cite{Oss92});
silicates and graphites (Sil-Dl and grf-DL) from Draine \& Lee (\cite{Dra84}),
amorphous carbon (amC-Hn) from Hanner (\cite{Han88}) and SiC (SiC-Pg) from 
P\'egouri\'e (\cite{Peg88}). $^{*}$ IRAS~12584--4837 (Hen3--847), IRAS~18062+2410 (SAO~85766) and 
IRAS~18379--1707 (LSS~5112) are variable in $J$, $H$, $K$ bands (see Table 3a). Hence, two separate 
models satisfied the warm dust component in IRAS~12584--4837 (Hen3--847). Model 1 conforms to the $J$, $H$, $K$ data from
Fouque et~al. (\cite{Fou92}). Model 2 conforms to the $J$, $H$, $K$ data from the 2MASS catalog. 
\end{table}