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20092025
most citedCarbon-enhanced metal-poor stars: the most pristine objects?

160 citations · 1.1k across the 24 of their papers we have counts for

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Showing 2013Show all

6 papers · 1 filter

astro-ph.SR2013★ 70 cited

TOPoS: I. Survey design and analysis of the first sample

E. Caffau, P. Bonifacio, L. Sbordone +14

The metal-weak tail of the metallicity distribution function (MDF) of the Galactic Halo stars contains crucial information on the formation mode of the first generation of stars. T…

astro-ph.GA2013★ 51 cited

X-Shooter GTO: evidence for a population of extremely metal-poor, alpha-poor stars

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

The extremely metal-poor stars are the direct descendants of the first generation stars. They carry the chemical signature of the pristine Universe at the time they formed, shortly…

astro-ph.SR2013★ 21 cited

Stellar granulation as seen in disk-integrated intensity. I. Simplified theoretical modeling

R. Samadi, K. Belkacem, H. -G. Ludwig

The solar granulation is known for a long time to be a surface manifestation of convection. Thanks to the current space-borne missions CoRoT and Kepler, it is now possible to obser…

astro-ph.SR2013★ 27 cited

The photospheric solar oxygen project: II. Non-concordance of the oxygen abundance derived from two forbidden lines

Elisabetta Caffau, Hans-G. Ludwig, Jean-M. Malherbe +3

In the Sun, the two forbidden [OI] lines at 630 and 636 nm were previously found to provide discrepant oxygen abundances. aims: We investigate whether this discrepancy is peculiar…

astro-ph.GA2013★ 160 cited

Carbon-enhanced metal-poor stars: the most pristine objects?

Monique Spite, E. Caffau, Piercarlo Bonifacio +4

Carbon-enhanced metal poor stars (CEMP) form a significant proportion of the metal-poor stars, their origin is not well understood. Three very metal-poor C-rich turnoff stars were…

astro-ph.SR2013★ 53 cited

Convective line shifts for the Gaia RVS from the CIFIST 3D model atmosphere grid

C. Allende Prieto, L. Koesterke, H. -G. Ludwig +2

To derive space velocities of stars along the line of sight from wavelength shifts in stellar spectra requires accounting for a number of second-order effects. For most stars, grav…