Free Access
Fig. 4
Spectra of the newly identified O/B type stars. The fluxes are normalised and an offset is added to the flux. The spectra are not shifted to rest wavelength. The numbers denote the identification numbers of the stars as listed in Tables B.1−B.3. We also show the S/N and denote probable foreground stars with “fg”.
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.