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Table 9:

Minimum and maximum equilibrium temperature and distribution of the dust mass with dust temperature ranges.
  NGC 1705 a Haro 11 a Mrk 1089
$T_{\rm eq}$$_{\rm (max)}$(K) 88.2 125 146
$T_{\rm eq}$$_{\rm (min)}$(K) 10 10 16.9
$f_{\rm mass}$([50 K; 150 K]) 0.1$\%$ 0.4$\%$ 0.15$\%$
$f_{\rm mass}$([25 K; 50 K]) 7.2$\%$ 28.9$\%$ 9.5$\%$
$f_{\rm mass}$([15 K; 25 K]) 8.3$\%$ 0$\%$ 90.4$\%$
$f_{\rm mass}$(10 K) 84.4$\%$ 70.4$\%$ 0$\%$

a The models used for NGC 1705 and Haro 11 include an independent, very cold dust component at 10 K with an emissivity $\beta $ = 1.


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