collaborators

7 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

Binary Constraints on the Origin of Nitrogen-rich Field Stars

Liao Yang, Baitian Tang, José G. Fernández-Trincado +5

Recent JWST observations have revealed galaxies with unusually high N/O ratios, suggesting that nitrogen enrichment may be common in intense star-forming environments in the early…

astro-ph.SR2026

Multiple populations detection with the Chinese Space Station Survey Telescope main survey camera

Zhuohang Li, Xia Li, Hao Tian +6

Multiple stellar populations (MPs), characterized by star-to-star light-element abundance variations, are ubiquitous in globular clusters (GCs). Spectroscopy directly reveals these…

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.GA2026

Spatial Property of Multiple Metallic Populations in the Tidal Stream of ω Centauri

Shiru Zheng, Baitian Tang, Long Wang +4

ω Centauri, the remnant nucleus of an accreted dwarf galaxy, is a unique laboratory for studying complex stellar populations. The recently discovered Fimbulthul stream provides a…

astro-ph.GA2026

A Tale of Two Origins: In-Situ versus Accreted Nitrogen-Rich Field Stars in the MW

Yi Qiao, Baitian Tang, José G. Fernández-Trincado +14

Spectroscopic surveys have identified significant numbers of metal-poor nitrogen-rich (N-rich) field stars. These stars are strong candidates for escapees from globular clusters (G…