Fig. 2
Upper panel: time evolution of Γ(M,EOS) for some stellar models evolving from the PMS to the WD stage. The mass range is 0.1–1.7 M⊙ (see symbols in the left upper corner). The adopted initial chemical composition is X = 0.73, Z = 0.01 and the mixing-length parameter αMLT = 1.5. Lower panel: specific nuclear power for the same models.
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.