activity
20242026
collaborators

10 papers

astro-ph.GA2026

Reconstructing the Stripping History of the Sagittarius Stream with Neural Networks

Jian Zhang, Cuihua Du, Mingji Deng +2

The Sagittarius (Sgr) Stream is produced by the ongoing disruption of the Sgr dwarf spheroidal (dSph) galaxy and is thought to contain multiple wraps that were stripped during diff…

astro-ph.GA2026

Revisiting candidate high-velocity stars associated with the Sagittarius dwarf spheroidal galaxy

Jian Zhang, Cuihua Du, Mingji Deng +2

Hypervelocity stars (HVSs) are valuable tracers of extreme dynamical processes. The Sagittarius dwarf spheroidal galaxy (Sgr dSph), currently undergoing tidal disruption, offers a…

astro-ph.GA2026

Chemical Properties and Sagittarius-induced Dynamical Perturbations of the GD-1 Stream

Haoyang Liu, Cuihua Du

In this study, we investigate the chemical properties of the GD-1 stream using cross-matched, data-driven elemental abundances. The results reveal no clear -knee in the [Mg/Fe]…

astro-ph.GA2026

A Low-mass Model of The Milky Way: The Disk Warp Resulting from A Galaxy Merger

Mingji Deng, Cuihua Du, Jian Zhang +2

Previous studies have shown that disk warps can result from galaxy mergers. Recent research indicates a noticeable decline in the rotation curve (RC) of the Milky Way (MW), suggest…

astro-ph.GA2025

Kinematic, Elemental and Structural Dependences on Metallicity in the Galactic Bulge

Haoyang Liu, Cuihua Du, Zhongcheng Li +2

We selected Bulge stars from APOGEE DR17 cross-matched with astrometric data from \textit{Gaia} DR3. Bulge stars were divided into sub-samples with line-of-sight velocity dispersio…

astro-ph.GA2025

CNN-Derived Elemental Abundances of LAMOST DR10 Giants: Implications for Galactic Substructures

Haoyang Liu, Cuihua Du, Mingji Deng +1

Stellar parameters and abundances provide crucial insights into stellar and Galactic evolution studies. In this work, we developed a convolutional neural network (CNN) to estimate…