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19962024
most citedFirst stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

1.2k citations · 13.3k across the 232 of their papers we have counts for

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astro-ph.SR2010★ 13 cited

The solar photospheric abundance of zirconium

Elisabetta Caffau, Rosanna Faraggiana, Hans-Günter Ludwig +2

Zirconium (Zr), together with strontium and yttrium, is an important element in the understanding of the Galactic nucleosynthesis. In fact, the triad Sr-Y-Zr constitutes the first…

astro-ph.GA2010★ 1 cited

Is Palomar 1 really associated with the Canis Major overdensity?

Ivo Saviane, Lorenzo Monaco, Matteo Correnti +2

It has recently been suggested that the peculiar cluster Pal 1 is associated to the Canis Major dwarf galaxy, which existence is still at the center of a debate. Our first measurem…

astro-ph.GA2010★ 45 cited

Li - O anti-correlation in NGC 6752: evidence for Li-enriched polluting gas

Z. -X. Shen, P. Bonifacio, L. Pasquini +1

Elemental correlations and anti-correlations are known to be present in globular clusters (GCs) owing to pollution by CNO cycled gas. Because of its fragility Li is destroyed at th…

astro-ph.IM2010★ 2 cited

GYES, a multifibre spectrograph for the CFHT

P. Bonifacio, S. Mignot, J. -L. Dournaux +38

We have chosen the name of GYES, one of the mythological giants with one hundred arms, offspring of Gaia and Uranus, for our instrument study of a multifibre spectrograph for the p…

astro-ph.SR2010★ 15 cited

Cu I resonance lines in turn-off stars of NGC 6752 and NGC 6397. Effects of granulation from CO5BOLD models

Piercarlo Bonifacio, Elisabetta Caffau, Hans-Günter Ludwig

Context. Copper is an element whose interesting evolution with metallicity is not fully understood. Observations of copper abundances rely on a very limited number of lines, the st…

astro-ph.GA2010

Local stars formed at z>10: a sample extracted from the SDSS

Luca Sbordone, Piercarlo Bonifacio, Elisabetta Caffau +1

As the Universe emerged from its initial hot and dense phase, its chemical composition was extremely simple, being limited to stable H and He isotopes, and traces of Li. The first…