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Faint population III supernovae as the origin of the most iron-poor stars

Astrophysical Journal Letters (2014) 792(2)
DOI: 10.1088/2041-8205/792/2/L32
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Abstract

The most iron-poor stars in the Milky Way provide important observational clues to the astrophysical objects that enriched the primordial gas with heavy elements. Among them, the recently discovered iron-deficient star SMSS J031300.36-670839.3 shows a remarkable chemical composition with a non-detection of iron ([Fe/H]

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Ishigaki, M. N., Tominaga, N., Kobayashi, C., & Nomoto, K. (2014). Faint population III supernovae as the origin of the most iron-poor stars. Astrophysical Journal Letters, 792(2). https://doi.org/10.1088/2041-8205/792/2/L32

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