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

Ishigaki, Miho N., Tominaga, Nozomu, Kobayashi, Chiaki and Nomoto, Ken'ichi (2014) Faint Population III supernovae as the origin of the most iron-poor stars. Astrophysical Journal Letters, 792 (2). ISSN 2041-8205

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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]$

Item Type	Article
Identification Number	10.1088/2041-8205/792/2/L32
Additional information	The Astrophysical Journal Letters, 792:L32 (6pp), 2014 September 10. doi: 10.1088/2041-8205/792/2/L32. © 2014 The American Astronomical Society. All rights reserved. Printed in the U.S.A.
Keywords	stars: abundances, stars: population iii, supernovae: general
Date Deposited	15 May 2025 13:11
Last Modified	31 Jan 2026 00:02