Trans-Fe elements from type Ia supernovae - I. Heavy element nucleosynthesis during the formation of near-Chandrasekhar white dwarfs

Open Access

Fig. 11.

Final mass fraction abundances of ⁸⁶Kr, ⁸⁷Rb, ⁸⁸Sr, ⁸⁹Y, and ⁹⁰Zr in the external layers of Model D, employing different ²²Ne(α,n)²⁵Mg and ²²Ne(α,γ)²⁶Mg nuclear reaction rates. See main text for details.

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.