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Table 3

Source parameters for the DUSTY fit.

Free Parameters

Source Rint Rint/ Luminosity Tstar Tdust Rout/ τV Grains Mdust
[arcsec] [104] [103L] [K] [K] composition [10-4M]

NGC 6369 ........ 2.8(±0.2)  200(±20) 3 70 000 140(±4) 100 0.030(±0.001) am-C 4(±3)
NGC 6572 ........ 3.7(±0.3)  180(±20) 8.3 80 000 160(±5) 30 0.013(±0.001) am-C 0.7(±0.3)
Helix .......... 140(±20) 22 000(±4000) 0.12 110 000 34(±2) 20 0.0085(±0.0001) am-C 18(±7)
NGC 7009 ........ 6.0(±0.4)  300(±20) 5 80 000 115(±3) 100 0.0029(±0.0001) Sil-DL 2(±1)
NGC 6720 ........ 4.8(±0.4) 2400(±200) 0.2 120 000 80(±3) 200 0.035(±0.002) am-C 11(±5)
NGC 6826 ........ 2.3(±0.2)  100(±10) 1.64 47 500 120(±5) 30 0.030(±0.002) Sil-DL 1.5(±0.6)
NGC 7027 ........ 2.6(±0.1)  580(±20) 10 190 000 190(±2) 200 0.025(±0.004) am-C 4(±2)
NGC 6543 ........ 4.8(±0.5)  130(±10) 5.2 56 000 120(±5) 100 0.012(±0.001) Sil-DL 6(±3)
NGC 40 ........ 2.3(±0.2)  74(±6) 1.7 50 000 160(±5) 100 0.040(±0.002) am-C 2(±1)
CRL 618 ........ 0.29(±0.03) 2.0(±0.2) 6 30 000 450(±4) 10 000 50(±4) am-C 4 000(±2 000)
IC 418 ........ 2.5(±0.3)  20(±2) 10 35 000 200(±8) 200 0.040(±0.001) am-C 6(±3)
NGC 3242 ........ 0.8(±0.2) 80(±20) 0.6 80 000 200(±20) 100 0.007(±0.001) Sil-Ow 0.3(±0.2)

Notes. Am-C indicates amorphous carbon (Hanner 1988), Sil-Ow indicate O-deficient silicates (Ossenkopf et al. 1992), and Sil-DL are astronomical silicates (Draine & Lee 1984).

(†)

To estimate the errors on the input and output parameters the DUSTY code has been used by varying arbitrarily this parameter by a factor of two.

(††)

Rc indicates the radius of the central star.

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