Open Access
Fig. B.1.
Download original image
Same as Fig. 1 but now comparing the results generated using MIST and Stromlo stellar tracks to show the dependence on initial metal abundances at a given metallicity. The tracks shown here are for two metallicities, [Fe/H]= − 1 and −2, and for non-rotating stars with highly clumped, close to optically thin winds.
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.