Figure 9 from The Inner 25 au Debris Distribution in the ϵ Eri System

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The Inner 25 au Debris Distribution in the ϵ Eri System

Authors: Kate Y. L. Su, James M. De Buizer, George H. Rieke, Alexander V. Krivov, Torsten Löhne, Massimo Marengo, Karl R. Stapelfeldt, Nicholas P. Ballering, and William D. Vacca

2017 The Astronomical Journal 153 226.

Provider: AAS Journals

Caption: Figure 9.

Model results using the geometric parameters of Greaves et al. (2014) in comparison with the observed disk profile (upper panel) and SED (lower panel). Symbols and lines are the same as in Figure 8. In the bottom SED plot, the model SED for the puffed-up dust disk is shown as the red solid line and the broad cold disk is shown as the brown solid line with the sum shown as the black dashed line.

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