Free Access

Fig. 3


Kippenhahn diagrams for our stellar evolution models. Models in the left column are computed without pulsation-driven mass loss (ε = 0) and those in the right column include pulsation-driven mass loss with ε = 0.1. The initial masses of the models are 150 (top), 200 (middle), and 250 M (bottom).

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.