A synthetic population of Wolf-Rayet stars in the LMC based on detailed single and binary star evolution models

Open Access

Fig. C.1.

Phase diagram of binary models with a fixed initial donor mass of M_1, i = 31.6 M_⊙. The initial mass ratio q_i is plotted versus the initial orbital period P_i. The different phases are indicated in the legend and a more detailed description can be found in the text.

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.