Fig. 2
Top: LABOCA observations towards R Scl. The colour scale is given in Jy beam−1. Middle: LABOCA map with the stellar SED (retrieved from the ALMA continuum observations convolved by the LABOCA beam) subtracted. Bottom: residual map after subtracting the stellar SED and a spherical detached shell with a radius of 18′′.5 and width of 2′′. The structures in the residual map are due to asymmetric emission from the shell, consistent with scattered-light observations.
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