activity
19942008
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 · 2k across the 23 of their papers we have counts for

collaborators
Showing 2008Show all

5 papers · 1 filter

astro-ph200831 cited

Stellar abundances and ages for metal-rich Milky Way globular clusters - Stellar parameters and elemental abundances for 9 HB stars in NGC6352

S. Feltzing, F. Primas, R. A. Johnson

[ABRIDGED] Metal-rich globular clusters provide important tracers of the formation of our Galaxy. Moreover, and not less important, they are very important calibrators for the deri…

astro-ph200897 cited

Galactic abundance gradients from Cepheids : On the iron abundance gradient around 10-12 kpc

B. Lemasle, P. Francois, A. Piersimoni +5

Context: Classical Cepheids can be adopted to trace the chemical evolution of the Galactic disk since their distances can be estimated with very high accuracy. Aims: Homogeneous ir…

astro-ph2008227 cited

The influence of chemical composition on the properties of Cepheid stars. II-The iron content

M. Romaniello, F. Primas, M. Mottini +6

The Cepheid period-luminosity (PL) relation is unquestionably one of the most powerful tools at our disposal for determining the extragalactic distance scale. While significant pro…

astro-ph20082 cited

The ESO Large Programme First Stars

P. Bonifacio, J. Andersen, S. Andrievsky +19

In ESO period 65 (April-September 2000) the large programme 165.N-0276, led by Roger Cayrel, began making use of UVES at the Kueyen VLT telescope. Known within the Team and outside…

astro-ph200826 cited

Possible signature of hypernova nucleosynthesis in a beryllium rich halo dwarf

R. Smiljanic, L. Pasquini, F. Primas +3

As part of a large survey of halo and thick disc stars, we found one halo star, HD 106038, exceptionally overabundant in beryllium. In spite of its low metallicity, [Fe/H] = -1.26,…