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20022007
most citedUncovering the Chemical Signature of the First Stars in the Universe

126 citations · 174 across the 2 of their papers we have counts for

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astro-ph2007126 cited

Uncovering the Chemical Signature of the First Stars in the Universe

Torgny Karlsson, Jarrett L. Johnson, Volker Bromm

The chemical abundance patterns observed in metal-poor Galactic halo stars contain the signature of the first supernovae, and thus allows us to probe the first stars that formed in…

astro-ph200648 cited

Primordial Stellar Feedback and the Origin of Hyper Metal-Poor Stars

Torgny Karlsson

The apparent absence of stars in the Milky Way halo with -5 ~< [Fe/H] ~< -4 suggests that the gas out of which the halo stars were born experienced a period of low or delayed star…

astro-ph2005

Stochastic chemical enrichment in metal-poor systems II. Abundance ratios and scatter

T. Karlsson, B. Gustafsson

A stochastic model of the chemical enrichment of metal-poor systems by core-collapse supernovae is used to study the scatter in stellar abundance ratios. The resulting scatter in a…

astro-ph2005

Stochastic chemical enrichment in metal-poor systems I. Theory

T. Karlsson

A stochastic model of the chemical enrichment of metal-poor systems by core-collapse (Type II) supernovae is presented, allowing for large-scale mixing of the enriched material by…

astro-ph2004

Abundances In Very Metal Poor Dwarf Stars

Judith G. Cohen, Norbert Christlieb, Andrew McWilliam +7

We discuss the detailed composition of 28 extremely metal-poor dwarfs, 22 of which are from the Hamburg/ESO Survey, based on Keck Echelle spectra. Our sample has a median [Fe/H] of…

astro-ph2003

HE0107-5240, A Chemically Ancient Star.I. A Detailed Abundance Analysis

N. Christlieb, B. Gustafsson, A. J. Korn +5

We report a detailed abundance analysis for HE0107-5240, a halo giant with [Fe/H]_NLTE=-5.3. This star was discovered in the course of follow-up medium-resolution spectroscopy of e…