activity
20012026
most citedThe sensitivity of Lick indices to abundance variations

134 citations · 526 across the 10 of their papers we have counts for

collaborators

10 papers

astro-ph.SR2026

gr8stars II : judgement day for spectroscopic parameter model systematics

Alix Violet Freckelton, Annelies Mortier, Megan Bedell +18

Many areas of astrophysics, including exoplanetary studies, rely on precise and accurate stellar parameters. This demands that uncertainties on these parameters truly reflect all b…

astro-ph.SR2023

Atomic Diffusion and Mixing in Old Stars VIII: Chemical abundance variations in the globular cluster M4 (NGC 6121)

T. Nordlander, P. Gruyters, O. Richard +1

Variations in chemical abundances with evolutionary phase have been identified among stars in globular and open clusters with a wide range of metallicities. In the metal-poor clust…

astro-ph.GA2019

4MOST Consortium Survey 2: The Milky Way Halo High-Resolution Survey

N. Christlieb, C. Battistini, P. Bonifacio +19

We will study the formation history of the Milky Way, and the earliest phases of its chemical enrichment, with a sample of more than 1.5 million stars at high galactic latitude. El…

astro-ph.SR2013★ 65 cited

Atomic diffusion and mixing in old stars IV: Weak abundance trends in the globular cluster NGC 6752

Pieter Gruyters, Andreas J. Korn, Olivier Richard +5

Atomic diffusion in stars can create systematic trends of surface abundances with evolutionary stage. Globular clusters offer useful laboratories to put observational constraints o…

astro-ph.SR2012★ 66 cited

Atomic Diffusion and Mixing in Old Stars. III. Analysis of NGC 6397 Stars under New Constraints

T. Nordlander, A. J. Korn, O. Richard +1

We have previously reported on chemical abundance trends with evolutionary state in the globular cluster NGC 6397 discovered in analyses of spectra taken with FLAMES at the VLT. He…

astro-ph.SR2009★ 28 cited

HE 1327-2326, an unevolved star with [Fe/H] < -5.0 III. Does Its Atmosphere Reflect Its Natal Composition?

A. J. Korn, O. Richard, L. Mashonkina +3

Based on spectroscopic constraints derived from NLTE line formation, we explore the likely range of stellar parameters (T_eff and log g) for the hyper-metal-poor (HMP) star HE 1327…