Free Access
Fig. 13
Hertzsprung-Russell diagram showing two pulsating late-type Be stars in comparison with HD 50138. Parameters of the Be stars are from Neiner et al. (2009) and Diago et al. (2009). Solid lines encompass the main sequence, dashed lines represent the evolutionary tracks for stars with MZAMS = 4 and 5 M⊙.
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.