Fig. 2
Left: SED of MWC 922 as in CSC+17, after adding PACS and SPIRE data (Molinari et al. 2016; Ramos-Medina et al. 2018), and including our ALMA continuum flux measurements (cyan, Table 1). Right: ALMA millimeter-continuum fluxes before (black) and after (blue) subtraction of the ~162 K dust emission contribution (dotted line in left panel). The red stars represent single-dish IRAM-30 m data (CSC+17).
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