Nova contributions to the chemical evolution of the Milky Way

Open Access

Fig. 21.

Bar plot summarising the contributions to each isotope by [Fe/H] = 0 for each nova yield profile, distinguishing between nova progenitor WD masses. Figs. A.1, A.2, and A.3 present the full evolution history for each isotope, also distinguishing progenitor masses.

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.