Fig. 3

Graphical explanation of the BCD spectrophotometric parameters (D,λ1,Φb,Φuv). In a) the determination of the BCD parameters is shown for a star in a B-normal type phase; b) displays a Be star whose second component of the Balmer discontinuity is in emission (flux excess); c) is for a Be-shell phase where the second component of the Balmer discontinuity appears in absorption (flux deficiency). The parameter D∗ (heavy full line) that measures the photospheric component of the Balmer discontinuity is given in dex, while the average spectral position of the Balmer discontinuity is generally given in λ1−3700 Å. In stars with a second component in emission or in absorption the parameter Φuv is generally not measured.
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.