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20002021
most citedFirst stars V - Abundance patterns from C to Zn and supernova yields in the early Galaxy

1.2k citations · 5.2k across the 42 of their papers we have counts for

collaborators

41 papers

astro-ph.SR2021★ 10 cited

Metal-Poor Stars Observed with the Southern African Large Telescope II. An Extended Sample

Joseph Zepeda, Kaitlin C. Rasmussen, Timothy C. Beers +3

We present results from high-resolution (R ) spectroscopic observations of over 200 metal-poor stars, mostly selected from the RAVE survey, using the Southern African…

astro-ph.SR2021

Barium lines in high-quality spectra of two metal-poor giants in the Galactic halo

G. Cescutti, C. Morossi, M. Franchini +9

Context. Theoretical results showed the possibility that neutron capture elements were produced in the early Universe by two different sources: a frequent s-process source hosted b…

astro-ph.GA2021

UVES analysis of red giants in the bulge globular cluster NGC 6522

B. Barbuy, E. Cantelli, L. Muniz +10

NGC 6522 is a moderately metal-poor bulge globular cluster ([Fe/H]1.0), and it is a well-studied representative among a number of moderately metal-poor blue horizontal bra…

astro-ph.SR2020★ 21 cited

Metal-Poor Stars Observed with the Southern African Large Telescope

Kaitlin C. Rasmussen, Joseph Zepeda, Timothy C. Beers +5

We present the first release of a large-scale study of relatively bright (V < 13.5) metal-poor stars observed with the Southern African Large Telescope (SALT), based on high-resolu…

astro-ph.SR2018★ 80 cited

Binarity among CEMP-no stars: an indication of multiple formation pathways?

Anke Arentsen, Else Starkenburg, Matthew D. Shetrone +3

Carbon-enhanced metal-poor (CEMP) stars comprise a large percentage of stars at the lowest metallicities. The stars in the CEMP-no subcategory do not show any s-process enhancement…

astro-ph.SR2017★ 108 cited

PLATO as it is: a legacy mission for Galactic archaeology

A. Miglio, C. Chiappini, B. Mosser +102

Deciphering the assembly history of the Milky Way is a formidable task, which becomes possible only if one can produce high-resolution chrono-chemo-kinematical maps of the Galaxy.…