activity
20002023
most citedMeasurement of stellar age from uranium decay

381 citations · 1.6k across the 13 of their papers we have counts for

collaborators

13 papers

astro-ph.GA2023★ 20 cited

Extremely metal-poor stars in the Fornax and Carina dwarf spheroidal galaxies

R. Lucchesi, P. Jablonka, Á. Skúladóttir +6

We present our analysis of VLT/UVES and X-shooter observations of six very metal-poor stars, including four stars at [Fe/H] in the Fornax and Carina dwarf spheroidal (…

astro-ph.GA2012★ 122 cited

A primordial star in the heart of the Lion

E. Caffau, P. Bonifacio, P. François +14

Context: The discovery and chemical analysis of extremely metal-poor stars permit a better understanding of the star formation of the first generation of stars and of the Universe…

astro-ph.SR2011★ 18 cited

Extremely metal-poor stars in SDSS fields

Piercarlo Bonifacio, Elisabetta Caffau, Patrick François +12

Some insight on the first generation of stars can be obtained from the chemical composition of their direct descendants, extremely metal-poor stars (EMP), with metallicity less tha…

astro-ph.SR2011★ 53 cited

First stars XIII. Two extremely metal-poor RR Lyrae stars?

C. J. Hansen, B. Nordstroem, P. Bonifacio +11

The chemical composition of extremely metal-poor stars (EMP stars; [Fe/H]<~ -3) is a unique tracer of early nucleosynthesis in the Galaxy. As such stars are rare, we wish to find c…

astro-ph.GA2010★ 117 cited

Non-LTE abundances of Mg and K in extremely metal-poor stars and the evolution of [O/Mg], [Na/Mg], [Al/Mg] and [K/Mg] in the Milky Way

S. M. Andrievsky, Monique Spite, S. A. Korotin +5

LTE abundances of light elements in extremely metal-poor (EMP) stars have been previously derived from high quality spectra. New derivations, free from the NLTE effects, will bette…

astro-ph.GA2009★ 83 cited

VLT-FLAMES Analysis of 8 giants in the Bulge Metal-poor Globular Cluster NGC 6522: Oldest Cluster in the Galaxy?

B. Barbuy, M. Zoccali, S. Ortolani +5

NGC 6522 has been the first metal-poor globular cluster identified in the bulge by W. Baade. Despite its importance, very few high resolution abundance analyses of stars in this cl…