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19982019
most citedFirst stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

1.2k citations · 7.4k across the 63 of their papers we have counts for

collaborators

63 papers

astro-ph.SR2019★ 17 cited

The Li/Li isotopic ratio in the metal-poor binary CS22876--032

J. I. González Hernández, P. Bonifacio, E. Caffau +4

We present high-resolution and high-quality UVES spectroscopic data of the metal-poor double-lined spectroscopic binary CS 22876--032 ([Fe/H] dex), with the goal to der…

astro-ph.SR2018★ 10 cited

TOPoS V: Abundance ratios in a sample of very metal-poor turn-off stars

P. François, E. Caffau, P. Bonifacio +12

Extremely metal-poor stars are keys to understand the early evolution of our Galaxy. The ESO large programme TOPoS has been tailored to analyse a new set of metal-poor turn-off sta…

astro-ph.SR2018★ 12 cited

Using the CIFIST grid of CO5BOLD 3D model atmospheres to study the effects of stellar granulation on photometric colours. II. The role of convection accross the H-R diagram

A. Kučinskas, J. Klevas, H. -G. Ludwig +3

We studied the influence of convection on the spectral energy distributions, photometric magnitudes, and colour indices of different types of stars across the H-R diagram. The 3D h…

astro-ph.SR2018★ 77 cited

TOPoS: IV. Chemical abundances from high-resolution observations of seven EMP stars

P. Bonifacio, E. Caffau, M. Spite +15

Extremely metal-poor stars provide us with indirect information on the first generations of massive stars. The TOPoS survey has been designed to increase the census of these stars…

astro-ph.SR2017★ 29 cited

Using the CIFIST grid of CO5BOLD 3D model atmospheres to study the effects of stellar granulation on photometric colours. I. Grids of 3D corrections in the UBVRI, 2MASS, Hipparcos, Gaia, and SDSS systems

P. Bonifacio, E. Caffau, H. -G. Ludwig +9

The atmospheres of cool stars are temporally and spatially inhomogeneous due to the effects of convection.The influence of this inhomogeneity, referred to as granulation, on colour…

astro-ph.GA2016★ 36 cited

TOPoS: III. An ultra iron-poor multiple CEMP system

E. Caffau, P. Bonifacio, M. Spite +15

One of the primary objectives of the TOPoS survey is to search for the most metal-poor stars. Our search has led to the discovery of one of the most iron-poor objects known, SDSS\,…