activity
20202026
most citedPurveyors of fine halos. II. Chemodynamical association of halo stars with Milky Way globular clusters

33 citations · 152 across the 16 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

9 papers · 1 filter

astro-ph.GA2026

Abundances of CNO in candidate young metal-poor stars

Piercarlo Bonifacio, Elisabetta Caffau, Luca Sbordone +6

In this contribution we investigate the CNO abundances in five apparently young evolved stars, with the aim of discriminating between truly young stars and stars that were rejuvena…

astro-ph.GA2026★ 1 cited

HR-GO II: chemical abundances of low- retrograde dynamically-tagged-groups: Revealing Thamnos as a very metal-poor substructure

Renjing Xie, Zhen Yuan, Haining Li +12

Milky Way halo substructures identified in dynamical space are known to suffer from contamination from the Milky Way in-situ stars, which makes their accreted origins uncertain. We…

astro-ph.GA2025★ 5 cited

MINCE III. Detailed chemical analysis of the UVES sample

F. Lucertini, L. Sbordone, E. Caffau +14

Context. The MINCE (Measuring at Intermediate Metallicity Neutron-Capture Elements) project aims to provide high quality neutron-capture abundances measurements in several hundred…

astro-ph.GA2024★ 10 cited

Chemical Evolution of R-process Elements in Stars (CERES). III. Chemical abundances of neutron capture elements from Ba to Eu

L. Lombardo, C. J. Hansen, F. Rizzuti +11

The chemical abundances of elements such as barium and the lanthanides are essential to understand the nucleosynthesis of heavy elements in the early Universe as well as the contri…

astro-ph.GA2024

HR-GO I: Comprehensive NLTE abundance analysis of the Cetus stream

T. M. Sitnova, Z. Yuan, T. Matsuno +8

Dwarf galaxy streams encode vast amounts of information essential to understanding early galaxy formation and nucleosynthesis channels. Due to the variation in the timescales of st…

astro-ph.GA2024★ 14 cited

High-speed stars. II. An unbound star, young stars, bulge metal-poor stars, and Aurora candidates

P. Bonifacio, E. Caffau, L. Monaco +6

The data from the Gaia satellite led us to revise our conception of the Galaxy structure and history. Hitherto unknown components have been discovered and a deep re-thinking of wha…

astro-ph.GA2022★ 27 cited

Chemical Evolution of R-process Elements in Stars (CERES). I. Stellar parameters and chemical abundances from Na to Zr

Linda Lombardo, Piercarlo Bonifacio, Patrick François +10

Aims. The Chemical Evolution of R-process Elements in Stars (CERES) project aims to provide a homogeneous analysis of a sample of metal-poor stars ([Fe/H]<-1.5). We present the ste…

astro-ph.GA2020

Purveyors of fine halos III. Chemical abundance analysis of a potential omega Cen associate

Andreas J. Koch-Hansen, Camilla Juul Hansen, Linda Lombardo +3

Globular clusters (GCs) are important donors to the build-up of the Milky Way (MW) stellar halo, having contributed at the ten percent level over the Galactic history. Stars that o…

astro-ph.GA2020★ 33 cited

Purveyors of fine halos. II. Chemodynamical association of halo stars with Milky Way globular clusters

Michael Hanke, Andreas Koch, Zdenek Prudil +2

We present chemodynamical links between the present-day Milky Way halo field star population and Galactic globular clusters (GCs) using a dataset that combines information from the…