Using results of nucleosynthesis calculations for theoretical core-collapse supernova models with various progenitor's masses, it is shown that abundance patterns of C, Mg, Si, Ca, and H seen in extremely metal-deficient stars with [Fe/H]
CITATION STYLE
Shigeyama, T., & Tsujimoto, T. (1998). Fossil Imprints of the First-Generation Supernova Ejecta in Extremely Metal-deficient Stars. The Astrophysical Journal, 507(2), L135–L139. https://doi.org/10.1086/311699
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