collaborators

10 papers

astro-ph.GA2026

Chemical Abundances and Globular Clusters of Milky Way Dwarf Galaxies

Baitian Tang, Shihui Lin, Ruoyun Huang +5

We present an overview of our ongoing GASTRONOMI project, which investigates the coevolution of the Milky Way (MW), its satellite dwarf galaxies, and their star clusters through ch…

astro-ph.GA2026

Milky Way Mapper decoded abundances -- II: From patterns to paths

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

The element abundances of Milky Way disc stars encode entangled imprints of multiple enrichment processes, making it difficult to uncover the underlying chemical evolution. Here we…

astro-ph.GA2026

Milky Way Mapper decoded abundances -- I. Shared disc enrichment patterns

Melissa K. Ness, Sarah Aquilina, Jennifer Mead +15

Elemental abundances in the Milky Way disc trace its star-formation and enrichment history, but predicting these abundances from theory is limited by uncertain nucleosynthetic yiel…

astro-ph.GA2026

APOGEE chemical abundances of stars in the MW satellites Fornax, Sextans, Draco and Carina

Cheng Xu, Yi Qiao, Baitian Tang +3

During its evolution, the Milky Way (MW) incorporated numerous dwarf galaxies, particularly low-mass systems. The surviving dwarf galaxies orbiting the MW serve as exceptional labo…

astro-ph.GA2025

SDSS-V LVM: Resolving Physical Conditions in the Trifid Nebula

Natascha Sattler, J. Eduardo Méndez-Delgado, Kathryn Kreckel +18

The chemical abundance of the interstellar medium sets the initial conditions for star formation and provides a probe of chemical galaxy evolution models. However, unresolved inhom…

astro-ph.SR2025

SPYGLASS. VII-A. The Demographics and Ages of Small Nearby Young Associations

Ronan Kerr, Facundo Peŕez Paolino, Jonathan C. Tan +5

Recent Gaia-based young stellar association surveys have revealed dozens of low-mass populations that have, until recently, been too small or sparse to detect. These populations re…