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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 4.

Excess-only profiles of the ϵ Eri system at 34.8 μm after photospheric subtraction (nominal and ±6.3% the photospheric values. The PSF profile (normalized to the peak) is shown as the dashed line. The excess emission is resolved at 34.8 μm, which could arise from (1) a central broad ring with a width of ∼18 au, shown as the green line, or (2) one point source plus a ring peaked at 10 au (not shown, see details in Section 4.2).

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