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

Miho N. Ishigaki; Nozomu Tominaga; Chiaki Kobayashi; Ken'ichi Nomoto

doi:10.1088/2041-8205/792/2/L32

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

Miho N. Ishigaki
, Nozomu Tominaga
, Chiaki Kobayashi
, Ken'ichi Nomoto

Research output: Contribution to journal › Article › peer-review

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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]$

Original language	English
Number of pages	6
Journal	Astrophysical Journal Letters
Volume	792
Issue number	2
DOIs	https://doi.org/10.1088/2041-8205/792/2/L32
Publication status	Published - 26 Aug 2014

Keywords

stars: abundances
stars: Population III
supernovae: general

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10.1088/2041-8205/792/2/L32

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title = "Faint Population III supernovae as the origin of the most iron-poor stars",

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]\$",

keywords = "stars: abundances, stars: Population III, supernovae: general",

author = "Ishigaki, \{Miho N.\} and Nozomu Tominaga and Chiaki Kobayashi and Ken'ichi Nomoto",

note = "The Astrophysical Journal Letters, 792:L32 (6pp), 2014 September 10. doi: 10.1088/2041-8205/792/2/L32. {\textcopyright} 2014 The American Astronomical Society. All rights reserved. Printed in the U.S.A.",

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AU - Ishigaki, Miho N.

AU - Tominaga, Nozomu

AU - Kobayashi, Chiaki

AU - Nomoto, Ken'ichi

PY - 2014/8/26

Y1 - 2014/8/26

N2 - 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]$

AB - 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]$

KW - stars: abundances

KW - stars: Population III

KW - supernovae: general

U2 - 10.1088/2041-8205/792/2/L32

DO - 10.1088/2041-8205/792/2/L32

M3 - Article

SN - 2041-8205

VL - 792

JO - Astrophysical Journal Letters

JF - Astrophysical Journal Letters

IS - 2

ER -

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

Abstract

Keywords

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