Free Access
Fig. 1
Predicted mass-loss rates for solar metallicity as a function of the stellar luminosity. Overplotted (solid line) is the fit to main-sequence O star mass-loss rates (Krtička & Kubát 2012). The dashed line denotes the one-line mass-loss rate estimate (Krtička & Kubát 2009a).
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.