Faint Population III supernovae as the origin of the most iron-poor stars
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Author
Ishigaki, Miho N.
Tominaga, Nozomu
Kobayashi, Chiaki
Nomoto, Ken'ichi
Attention
2299/19372
Abstract
The most iron-deficient stars in the Milky Way provide important observational constraints on the nature of astrophysical objects that have enriched the primordial gas with heavy elements from which these stars were formed. Among them, the recently discovered iron-deficient star SMSS J031300.36-670839.3 shows a remarkable chemical composition with non-detection of iron ([Fe/H]$ H]$