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20002009
most citedNucleosynthetic signatures of the first stars

566 citations · 2.2k across the 14 of their papers we have counts for

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Showing 2005 · astro-phShow all

8 papers · 2 filters

astro-ph2005

The Oxygen Abundance of HE 1327-2326

Anna Frebel, Norbert Christlieb, John E. Norris +2

From a newly obtained VLT/UVES spectrum we have determined the oxygen abundance of HE 1327-2326, the most iron-poor star known to date. UV-OH lines yield a 1D LTE abundance of [O/F…

astro-ph2005

Afterglow spectrum of a gamma-ray burst with the highest known redshift z=6.295

N. Kawai, G. Kosugi, K. Aoki +25

Gamma-ray bursts (GRBs) and their afterglows have been proposed as an excellent probe to study the evolution of cosmic star formation, the reionization of the intergalactic medium,…

astro-ph2005

Rubidium and lead abundances in giant stars of the globular clusters M 13 and NGC 6752

David Yong, Wako Aoki, David L. Lambert +1

We present measurements of the neutron-capture elements Rb and Pb in five giant stars of the globular cluster NGC 6752 and Pb measurements in four giants of the globular cluster M…

astro-ph2005

Mg isotope ratios in giant stars of the globular clusters M 13 and M 71

David Yong, Wako Aoki, David L. Lambert

We present Mg isotope ratios in 4 red giants of the globular cluster M 13 and 1 red giant of the globular cluster M 71 based on spectra obtained with HDS on the Subaru Telescope. W…

astro-ph2005

HE1327-2326, an unevolved star with [Fe/H]<-5.0. I. A Comprehensive Abundance Analysis

W. Aoki, A. Frebel, N. Christlieb +17

We present the elemental abundances of HE1327-2326, the most iron-deficient star known, determined from a comprehensive analysis of spectra obtained with the Subaru Telescope High…

astro-ph2005

The Origins of Two Classes of Carbon-Enhanced, Metal-Poor Stars

S. G. Ryan, W. Aoki, J. E. Norris +1

We have compiled composition, luminosity, and binarity information for carbon-enhanced, metal-poor (CEMP) stars reported by recent studies. We divided the CEMP star sample into two…