The Isotopic Scaling model(West & Heger, 2013) provides a complete average isotopic decomposition for our Milky Way as a function of metallicity and it requires an initial Solar Abundance Decomposition as a starting point. The previous Solar Abundance decomposition work is not perfect(West & Heger, 2013), since Classical Novae abundances are ignored. My research intends to improve the current solar abundance decomposition by adding Classical Novae Abundance contribution, then to update the Isotopic Scaling model.
"Adding Classical Novae Contribution to the Isotopic Scaling model,"
Macalester Journal of Physics and Astronomy: Vol. 11:
1, Article 2.
Available at: https://digitalcommons.macalester.edu/mjpa/vol11/iss1/2