The grain types used for modelling the SEDs are
"warm'' (Sil-Ow) and "cold'' (Sil-Oc) silicates from Ossenkopf et al. (1992);
silicates and graphites (Sil-Dl and grf-DL) from Draine & Lee (1984),
amorphous carbon (amC-Hn) from Hanner (1988) and SiC (SiC-Pg) from
Pégourié (1988). * 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. (1992). Model 2 conforms to the J, H, K data from the 2MASS catalog.
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