HE 1327−2326, an Unevolved Star with [Fe/H] < −5.0. I. A Comprehensive Abundance Analysis | Zendy

Wako Aoki | Zendy; Anna Frebel | Zendy; N. Christlieb | Zendy; John E. Norris | Zendy; Timothy C. Beers | Zendy; Takeo Minezaki | Zendy; P. S. Barklem | Zendy; Satoshi Honda | Zendy; Masahide TakadaHidai | Zendy; M. Asplund | Zendy; Sean G. Ryan | Zendy; Stelios Tsangarides | Zendy; Kimmo Eriksson | Zendy; A. Steinhauer | Zendy; Constantine P. Deliyannis | Zendy; K. Nomoto | Zendy; M. Y. Fujimoto | Zendy; Hiroyasu Ando | Zendy; Yuzuru Yoshii | Zendy; Toshitaka Kajino | Zendy

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HE 1327−2326, an Unevolved Star with [Fe/H] < −5.0. I. A Comprehensive Abundance Analysis

Author(s) -

Wako Aoki,

Anna Frebel,

N. Christlieb,

John E. Norris,

Timothy C. Beers,

Takeo Minezaki,

P. S. Barklem,

Satoshi Honda,

Masahide TakadaHidai,

M. Asplund,

Sean G. Ryan,

Stelios Tsangarides,

Kimmo Eriksson,

A. Steinhauer,

Constantine P. Deliyannis,

K. Nomoto,

M. Y. Fujimoto,

Hiroyasu Ando,

Yuzuru Yoshii,

Toshitaka Kajino

Publication year - 2006

Publication title -

the astrophysical journal

Language(s) - English

Resource type - Journals

SCImago Journal Rank - 2.376

H-Index - 489

eISSN - 1538-4357

pISSN - 0004-637X

DOI - 10.1086/497906

Subject(s) - physics , subgiant , abundance (ecology) , astrophysics , stars , biology , globular cluster , ecology

We present the elemental abundances of HE1327-2326, the most iron-deficientstar known, determined from a comprehensive analysis of spectra obtained withthe Subaru Telescope High Dispersion Spectrograph.Comment: 53 pages, 14 figures, 10 tables, to appear in Ap

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