Free Access

Fig. 3


Comparison of predicted P v ionization fractions (blue dots) with ionization fractions derived from observations (Massa et al. 2003, crosses) at the point where the wind velocity is equal to half of its terminal value for LMC stars as a function of stellar effective temperature. The ionization fractions derived from observations were scaled by the ratio of mass-loss rate used to derive the observational fractions and our predicted mass-loss rate for LMC metallicity.

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.