activity
19962009
most citedFirst stars VI - Abundances of C, N, O, Li, and mixing in extremely metal-poor giants. Galactic evolution of the light elements

434 citations · 522 across the 9 of their papers we have counts for

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Showing 2008Show all

8 papers · 1 filter

astro-ph20086 cited

Overview of the lithium problem in metal-poor stars and new results on 6Li

Roger Cayrel, Matthias Steffen, Piercarlo Bonifacio +2

Two problems are discussed here. The first one is the 0.4 dex discrepancy between the 7Li abundance derived from the spectra of metal-poor halo stars on the one hand, and from Big…

astro-ph2008

Spectral analyses of three carbon-enhanced metal-poor stars

N. T. Behara, Piercarlo Bonifacio, Hans-Guenter Ludwig +3

We are conducting a high-resolution follow-up of candidate EMP stars extracted from the Sloan Digital Sky Survey (SDSS; York et al. 2000) using UVES at the VLT. Three of the progra…

astro-ph200827 cited

Extremely metal-poor stars from the SDSS

H. -G. Ludwig, P. Bonifacio, E. Caffau +3

We give a progress report about the activities within the CIFIST Team related to the search for extremely metal-poor stars in the Sloan Digital Sky Survey's spectroscopic catalog.…

astro-ph2008

True solar analogues in the open cluster M67

K. Biazzo, L. Pasquini, P. Bonifacio +2

The solar analogues are fundamental targets for a better understanding of our Sun and Solar System. Notwithstanding the efforts, this research is usually limited to field stars. Th…

astro-ph20083 cited

From Espresso to Codex

J. Liske, L. Pasquini, P. Bonifacio +24

CODEX and ESPRESSO are concepts for ultra-stable, high-resolution spectrographs at the E-ELT and VLT, respectively. Both instruments are well motivated by distinct sets of science…

astro-ph2008258 cited

Cosmic dynamics in the era of Extremely Large Telescopes

J. Liske, A. Grazian, E. Vanzella +24

The redshifts of all cosmologically distant sources are expected to experience a small, systematic drift as a function of time due to the evolution of the Universe's expansion rate…