Free Access

Fig. 2


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.

This figure is made of several images, please see below:

Current usage metrics show cumulative count of Article Views (full-text article views including HTML views, PDF and ePub downloads, according to the available data) and Abstracts Views on Vision4Press platform.

Data correspond to usage on the plateform after 2015. The current usage metrics is available 48-96 hours after online publication and is updated daily on week days.

Initial download of the metrics may take a while.