Fig. 4
Spectral energy distribution of IRAS 17150−3224 in black dots. The 8.5 and 10.0 μm points are from Ueta et al. (2000), the 12, 25, 60, and 100 μm points from IRAS, the 800.0 and 1100.0 μm points from Hu et al. (1993) and the 1.3 mm from Guertler et al. (1996). In grey is our model based on the parameters of Meixner et al. (2002).
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