University of Hertfordshire

From the same journal

From the same journal

By the same authors

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

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Original languageEnglish
Number of pages6
JournalAstrophysical Journal Letters
Volume792
Issue2
DOIs
Publication statusPublished - 26 Aug 2014

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]$

Notes

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.

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