Figure 3 from A PRIMER ON UNIFYING DEBRIS DISK MORPHOLOGIES

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A PRIMER ON UNIFYING DEBRIS DISK MORPHOLOGIES

Authors: Eve J. Lee, and Eugene Chiang

2016 The Astrophysical Journal 827 125.

Provider: AAS Journals

Caption: Figure 3.

Same as Figure 2, but for a more eccentric planet with ﹩{e}_{{\rm{planet}}}=0.7﹩. The surface brightnesses of the brightest features are ∼10⁴ (﹩2\times {10}^{4}﹩) times higher than that of the faintest features in the face-on (edge-on) view.

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