Table 3: Detailed results of the fits to the dust emission in two sources with two independent gray bodies (see text).
$T_{\rm w}$ $\tau_{30~{\rm w}}$ $\beta_{\rm w}$ $T_{\rm c}$ $\tau_{\rm 30~c}$ $\beta_{\rm c}$ $\chi^2$
M+0.76-0.05
25 0.27 1 13.9 101 3 162
25 0.27 1 14 16.8 2 158
25 0.27 1 15 1.83 1 157
24 0.60 1.5 15 6.3 1.5 166
24 0.63 1.5 14 59.6 2.5 168
23 1.63 2 13.4 58.1 2.0 180
23 1.70 2 13.2 174.3 2.5 170
M+0.21-0.12
41.8 0.035 1 16.8 0.70 1 37
41.6 0.036 1 14.6 9.04 2 38
41.3 0.038 1 13.4 91.2 3 40
38.6 0.082 1.5 15.4 18.9 2.5 44
39.0 0.076 1.5 17.5 1.68 1.5 40
36.0 0.183 2 16.7 6.17 2 41
35.6 0.203 2 15 63.6 3 47


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