Fig. 9
Comparison of our EPIC abundance measurements with standard SNe yield models. Left panel: WDD2 delayed-detonation SNIa model (Iwamoto et al. 1999). Right panel: empirically modified delayed detonation SNIa model from the yields of the Tycho supernova (Badenes et al. 2006). The two models are computed with a Salpeter IMF and an initial metallicity of Z = 0.02 (Nomoto et al. 2006).
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.