Original article can be found at: http://www.iop.org/EJ/journal/apj Copyright American Astronomical Society. DOI: 10.1086/512601 [Full text of this article is not available in the UHRA]Peer reviewe
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Original article can be found at: http://www.iop.org/EJ/journal/apj Copyright American Astronomical ...
detailed elemental abundance analysis has been carried out for the very metal-poor (Fe/H = -2.7)star...
We have obtained high-resolution (R ’ 50; 000 or 90,000), high-quality (S=Nk100) spectra of 22 very ...
A detailed elemental abundance analysis has been carried out for the very metal-poor ([Fe/H] = -2.7)...
A detailed elemental abundance analysis has been carried out for the very metal-poor ([Fe/H]=-2.7) s...
Original article can be found at: http://www.iop.org/ Copyright Royal Swedish Academy of Sciences [F...
The chemical abundances of large samples of extremely metal-poor (EMP) stars can be used to investig...
Elemental abundance measurements have been obtained for a sample of 18 very metal-poor stars using s...
The chemical abundances of very metal-poor stars provide important constraints on the nucleosynthesi...
Elemental abundance measurements have been obtained for a sample of 18 very metal-poor stars using s...
We analyze a high-resolution, high signal-to-noise ratio spectrum of the carbon-rich, extremely meta...
We analyze a high-resolution, high signal-to-noise ratio spectrum of the carbon-rich, extremely meta...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Original article can be found at: http://www.iop.org/EJ/journal/apj Copyright American Astronomical ...
detailed elemental abundance analysis has been carried out for the very metal-poor (Fe/H = -2.7)star...
We have obtained high-resolution (R ’ 50; 000 or 90,000), high-quality (S=Nk100) spectra of 22 very ...
A detailed elemental abundance analysis has been carried out for the very metal-poor ([Fe/H] = -2.7)...
A detailed elemental abundance analysis has been carried out for the very metal-poor ([Fe/H]=-2.7) s...
Original article can be found at: http://www.iop.org/ Copyright Royal Swedish Academy of Sciences [F...
The chemical abundances of large samples of extremely metal-poor (EMP) stars can be used to investig...
Elemental abundance measurements have been obtained for a sample of 18 very metal-poor stars using s...
The chemical abundances of very metal-poor stars provide important constraints on the nucleosynthesi...
Elemental abundance measurements have been obtained for a sample of 18 very metal-poor stars using s...
We analyze a high-resolution, high signal-to-noise ratio spectrum of the carbon-rich, extremely meta...
We analyze a high-resolution, high signal-to-noise ratio spectrum of the carbon-rich, extremely meta...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Context. The extremely metal-poor stars are the direct descendants of the first generation stars. Th...
Original article can be found at: http://www.iop.org/EJ/journal/apj Copyright American Astronomical ...