Fig. 12
Download original image
Coarse-grid models in the log Teff – log g diagram, chosen to be representative for hot dwarfs to “cool” supergiants in the O-star regime. Overplotted in green are evolutionary tracks for Galactic nonrotating stars from Ekström et al. (2012), and the blue line defines the corresponding ZAMS. The numbers give the initial stellar masses in units of 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.