Comparison of synthetic spectra (yellow dashed line) with the optical to radio SEDs of Cyg OB2 #12 (top panel), ζ1 Sco (middle panel) and HD 190603 (bottom panel). Note the lack of a near-mid IR excess signalling the absence of significant amounts (warm) circumstellar dust. Physical parameters employed in the modeling – such as Lbol and E(B − V) – may be found in Table 4 and Sects. 4.1 and 4.2.
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