The advanced evolution of massive stars - I. New reaction rates for carbon and oxygen nuclear reactions

Open Access

Fig. 5.

Profiles of abundances of ⁴He, ¹²C, ¹⁶O, ²⁰Ne, ²³Na, ²⁸Si, ³²S, ³⁴S, and ⁴⁴Ti (colour-coded) for a rotating 15 M_⊙, shown for different reaction rates scenarios distinguished by line style. Left panel: End of the C-burning phase. Right panel: End of the O-burning phase.

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.