Fig. 9
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Fractional width and radius of debris rings with non-edge-on geometries in Sco-Cen (circles). The circle sizes are proportionalto the disk fraction luminosity. HD 141011 (cross) falls in a void space close to the outer belt of HD 120326. The morphology of Fomalhaut inferred from optical (brown star, Kalas et al. 2005) or ALMA (yellow star, MacGregor et al. 2017)data are similar to those of HD 141011.
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