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Fig. 15
Modelled SED of the debris disk around HD 207129. From left to right: with 40%, 60%, and 80% of water ice in the dust material (the rest is astronomical silicate from Draine 2003). Compared are two models for the optical data of water ice: our model (at ϑ = 55 K) and the model of Li & Greenberg (1998).
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