Probing the dust properties of galaxies up to submillimetre wavelengths - I. The spectral energy distribution of dwarf galaxies using LABOCA

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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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