Francesca Primas

TL;DR: In this paper, high-resolution spectra obtained with three ground-based facilities and the Hubble Space Telescope (HST) have been combined to produce a new abundance analysis of CS 22892-052, an extremely metal-poor giant with large relative enhancements of neutron capture elements.

TL;DR: In this article, very high quality spectra of 24 metal-poor halo dwarfs and subgiants have been acquired with ESO's VLT/UVES for the purpose of determining Li isotopic abundances.

TL;DR: In this article, the structural parameters of the Fornax dwarf spheroidal galaxy were derived using wide field imaging covering the galaxy out to its tidal radius, and the spatial distribution of the stars of different ages as selected from colour-magnitude diagram analysis.

TL;DR: Cayrel et al. as discussed by the authors measured accurate, homogeneous neutron-capture element abundances for the sample of 32 EMP giant stars studied earlier in this series, including 22 stars with [Fe/H]< -3.5.

TL;DR: In this article, the authors compare the results for giants with new, accurate abundances for all observable elements in 18 extremely metal-poor (EMP) turnoff stars, at all metallicities.