collaborators

7 papers

astro-ph.GA2026

A -like metallicity profile in the disk of the Sagittarius dwarf galaxy

Zixi Guo, Xiang-Xiang Xue, Jiang Chang +12

Unveiling the properties of the progenitors that formed the tidal structures of the Milky Way (MW) is essential for exploring the MW's assembly history. Such studies further afford…

astro-ph.GA2026

Environmental Dependence of Satellite Planarity and Orbital-Pole Coherence around Milky Way Analogues in a Hydrodynamical Cosmological Simulation

Peng Wang, Yu Luo, Jiang Chang +2

We examine whether the unusual spatial flattening and orbital-plane coherence of the Milky Way's classical satellites are connected to the Galaxy's location in the cosmic web. We c…

astro-ph.CO2025

Particle loads for cosmological simulations with equal-mass dark matter and baryonic particles

Shihong Liao, Yizhou Liu, Haonan Zheng +5

Traditional cosmological hydrodynamical simulations usually assume equal-numbered but unequal-mass dark matter and baryonic particles, which can lead to spurious collisional heatin…

astro-ph.GA2025

A North-South Metallicity Asymmetry in the Outer Galactic disk -- Evidence for the Pericentric Passage of the Sagittarius Dwarf Galaxy

Chun Wang, Yang Huang, Timothy C. Beers +4

We present maps of the mean metallicity distributions on the Galactocentric -- plane at different azimuthal angles using red clump stars selected from the LAMOST and APOGEE s…

astro-ph.GA2025

ViT-based Local Volume dwarf galaxy Identificationin (VIDA) in the CSST survey

Han Qu, Zhen Yuan, Chengliang Wei +11

Identifying dwarf galaxies within the Local Volume is crucial for constraining the luminosity function of satellite galaxies in the nearby universe. We report the detection capabil…

astro-ph.GA2025

The Shape and Mass of the Galactic Dark Matter Halo from the Axisymmetric Jeans Model

Lan Zhang, Xiang-Xiang Xue, Ling Zhu +8

We explore the density profile, shape, and virial mass of the Milky Way's dark matter halo using K giants (KG) from LAMOST and SDSS/SEGUE, as well as blue horizontal branch (BHB) s…

astro-ph.GA2025

Where are the Population III star relics in the simulated Milky Way analogues?

Hang Yang, Liang Gao, Qi Guo +3

Using 6 Milky Way analogues with two different numerical resolutions from the Auriga simulation, we investigate the total mass, spatial distribution and kinematics of the Populatio…