JINA - Virtual Journal of Nuclear Astrophysics, 9 December 2022
Volume 20, Issue 48 (25 Articles)
- # 15 - Models for metal-poor stars with different initial abundances of C, N, O, Mg, and Si − III. Grids of isochrones for −2.5 ≤ [Fe/H] ≤ −0.5 and helium abundances Y = 0.25 and 0.29 at each metallicity
- Monthly Notices of the Royal Astronomical Society - Volume: 518, Issue: 3
- https://academic.oup.com/mnras/article/518/3/4517/6824455?rss=1