The study examines a very metal-poor star HE 2315−4240
Abundance ratio [X/H] of HE 2315−4240 (black filled circles) as a function of atomic number. Overplotted in green is the best-matched Population III nucleosynthesis model. The mass and energy of the model are shown in the upper right. Credit: Wang et al., 2024. Based on data from the Magellan-Clay telescope in Chile, astronomers have performed … Read more