chemical evolution 2galactic archaeology 2globular clusters 2magnesium isotopes 2stellar nucleosynthesis 2AGB stars 1chemical abundances 1dwarf galaxies 1high-resolution spectroscopy 1s-process enrichment 1stellar populations 1
From the 3 of 3 papers with an AI index.
29 citations
- ARC Centre of Excellence for All-sky AstrophysicsAU3 papers
- Australian National UniversityAU3 papers
- Monash UniversityAU3 papers
- UNSW SydneyAU3 papers
- Arcetri Astrophysical ObservatoryIT2 papers
- National Institute for AstrophysicsIT2 papers
- Osservatorio Astronomico di PadovaIT2 papers
- University of CambridgeGB2 papers
- University of PaduaIT2 papers
- Uppsala UniversitySE2 papers
- Aarhus UniversityDK1 paper
- Joint Institute for Nuclear AstrophysicsUS1 paper
3 papers
astro-ph.GA2026★ 5 cited
Magnesium isotope ratios in Milky Way and dwarf galaxy stars
M. McKenzie, S. Monty, D. Yong +8
The paper measures magnesium isotope ratios in stars from dwarf galaxies and the Milky Way, finding distinct patterns at fixed iron abundance but similar ratios at fixed magnesium…
astro-ph.GA2026★ 3 cited
The complex stellar system M 22: constraining the chemical enrichment from AGB stars using magnesium isotope ratios
M. McKenzie, D. Yong, A. I. Karakas +8
The paper measures magnesium isotope ratios in the globular‑cluster-like system M 22 and finds that low‑mass (1–3 M☉) AGB stars can explain its s‑process enrichment, while higher‑m…
astro-ph.GA2026★ 29 cited
The complex stellar system M 22: confirming abundance variations with high precision differential measurements
M. McKenzie, D. Yong, A. F. Marino +8
The authors perform high‑precision differential spectroscopy of six red‑giant stars in the globular‑cluster‑like system M 22, confirming internal abundance variations in many eleme…