activity
20232026
collaborators

6 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.GA2025

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.IM2024

A new code for low-resolution spectral identification of white dwarf binary candidates

Genghao Liu, Baitian Tang, Liangliang Ren +7

Close white dwarf binaries (CWDBs) are considered to be progenitors of several exotic astronomical phenomena (e.g., type Ia supernovae, cataclysmic variables). These violent events…

astro-ph.GA2024

Where do they come from? Identification of globular cluster escaped stars

Cheng Xu, Baitian Tang, Chengyuan Li +5

Globular clusters (GCs), as old as our Galaxy, constantly lose their members to the field as they cross through the Milky Way (MW). These GC escaped stars (or escapees) are suggest…

astro-ph.GA2023

Chemo-dynamical Nature of the Anticenter Stream and Monoceros Ring

Yi Qiao, Baitian Tang, Jianhui Lian +2

In the epoch of deep photometric surveys, a large number of substructures, e.g., over-densities, streams, were identified. With the help of astrometry and spectroscopy, the communi…

astro-ph.SR2023

The role of tidal interactions in the formation of slowly rotating early-type stars in young star clusters

Chenyu He, Chengyuan Li, Weijia Sun +9

The split main sequences found in the colour-magnitude diagrams of star clusters younger than ~600 Myr are suggested to be caused by the dichotomy of stellar rotation rates of uppe…