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 20 Aug 2026 23:01

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