Table 4: Input physical parameters for DUSTY and the adopted reddening values.
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)
12584-4837* warm1 0.27 0.18 20 000 amC-Hn 0.26 775
  warm2 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
$^{\dagger}$ 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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