Relative difference between the radiative flux of the ω-model and the ESTER model as a function of co-latitude for a 15 M⊙ (top) and a 40 M⊙ (bottom) ZAMS-star with various angular velocity ratios. The black line corresponds to an evolved 15 M⊙ ESTER 2D model with ω = 0.9 and a fractional abundance of hydrogen in the convective core Xcore/X0 = 0.5. X0 is the initial hydrogen mass fraction at ZAMS. The minimum of each curve corresponds to a sign change of FESTER − Fω.
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.