Free Access

Fig. 11


Averaged mass-loss rates of the WN stars in the SMC, LMC, MW, and the late type WN stars in M 31 plotted versus the iron abundance given in Table 1. The symbols are the same as in Fig. 1. The dashed line is a linear regression fit that is weighted by the number of objects analyzed in each galaxy.

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.