Fig. A.1.
Spectral energy distribution for R Hya using the continuum measurements obtained from Vizier (http://vizier.u-strasbg.fr/vizier/sed/) for a radius of 30″ (left panel), and 1″ (right panel), centred on the source. The flux density of the IRAS measurement at 100 microns (Hashimoto et al. 1998) and of our ALMA observation at 250 GHz are shown in red and blue, respectively.
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