activity
20122026
most citedA Low-Mass Stellar-Debris Stream Associated with a Globular Cluster Pair in the Halo

93 citations · 594 across the 19 of their papers we have counts for

collaborators
Showing astro-ph.GAShow all

17 papers · 1 filter

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

Disk tilts in Milky Way-like galaxies and their link to mergers

Runsheng Cai, Ling Zhu, Jiang Chang +3

We investigated disk reorientation and its relationship to mergers in a sample of 93 Milky Way-mass galaxies drawn from the TNG50 simulations. From this sample, we identified 117 i…

astro-ph.GA2026

The formation of the C-19 progenitor: a primordial cluster heated by gas expulsion

Zhen Wang, Long Wang, Zhen Yuan +1

The extremely metal-poor nature of the C-19 stream indicates that its progenitor was a primordial stellar system born in the very early Universe. Current observations show that it…

astro-ph.GA2023

Detection of multiple phase space overdensities of GSE stars by orbit integration

WenboWu, GangZhao, JiangChang +5

In N-body simulations, nearly radial mergers can form shell-like overdensities in the sky position and phase space () due to the combination of dynamical friction and tidal…

astro-ph.GA2022★ 15 cited

Local Group Dwarf Galaxy Detection Limit in the CSST survey

Han Qu, Zhen Yuan, Amandine Doliva-Dolinsky +9

We predict the dwarf galaxy detection limits for the upcoming Chinese Space Station Telescope (CSST) survey that will cover 17,500 deg of the sky with a wide field of view of…

astro-ph.GA2022★ 47 cited

LAMOST meets Gaia: The Galactic Open Clusters

Xiaoting Fu, Angela Bragaglia, Chao Liu +14

Open Clusters are born and evolve along the Milky Way plane, on them is imprinted the history of the Galactic disc, including the chemical and dynamical evolution. Chemical and dyn…

astro-ph.GA2021★ 39 cited

The Complexity of the Cetus Stream Unveiled from the Fusion of STREAMFINDER and StarGO

Zhen Yuan, Khyati Malhan, Federico Sestito +16

We combine the power of two stream-searching tools, STREAMFINDER and StarGO applied to the Gaia EDR3 data, to detect stellar debris belonging to the Cetus stream system that forms…

astro-ph.GA2020★ 21 cited

Discovery of A candidate Hypervelocity star originated from the Sagittarius Dwarf Spheroidal galaxy

Yang Huang, Qingzheng Li, Huawei Zhang +5

In this letter, we report the discovery of an intriguing HVS (J1443+1453) candidate that is probably from the Sagittarius Dwarf Spheroidal galaxy (Sgr dSph). The star is an old and…

astro-ph.GA2020★ 93 cited

A Low-Mass Stellar-Debris Stream Associated with a Globular Cluster Pair in the Halo

Zhen Yuan, Jiang Chang, Timothy C. Beers +1

There are expected to be physical relationships between the globular clusters (GCs) and stellar substructures in the Milky Way, not all of which have yet been found. We search for…

astro-ph.GA2020★ 30 cited

Is NGC 5824 the Core of the Progenitor of the Cetus Stream?

Jiang Chang, Zhen Yuan, Xiang-Xiang Xue +5

A large number of new members (150) of the Cetus Stream (CS) were identified from their clustering features in dynamical space using 6D kinematic data by combining LAMOST DR5…

astro-ph.GA2019★ 40 cited

Tracing Kinematic and Chemical Properties of Sagittarius Stream by K-Giants, M-Giants, and BHB stars

Chengqun Yang, Xiang-Xiang Xue, Jing Li +12

We characterize the kinematic and chemical properties of 3,000 Sagittarius (Sgr) stream stars, including K-giants, M-giants, and BHBs, select from SEGUE-2, LAMOST, and SDSS s…

astro-ph.GA2019★ 28 cited

Identifying Galactic Halo Substructure in 6D Phase-space Using 13,000 LAMOST K Giants

Chengqun Yang, Xiang-Xiang Xue, Jing Li +6

We construct a large halo K-giant sample by combining the positions, distances, radial velocities, and metallicities of over 13,000 LAMOST DR5 halo K giants with the Gaia DR2 prope…

astro-ph.GA2019★ 42 cited

Mapping the Galactic disk with the LAMOST and Gaia Red clump sample. II. 3D asymmetrical kinematics of mono-age populations in the disk between 6 \,kpc

H. -F. Wang, M. López-Corredoira, Y. Huang +11

We perform analysis of the three-dimensional kinematics of Milky Way disk stars in mono-age populations. We focus on stars between Galactocentric distances of and 14 \,kpc, s…

astro-ph.GA2019★ 35 cited

Revealing the Complicated Story of the Cetus Stream with StarGO

Zhen Yuan, M. C. Smith, Xiang-Xiang Xue +5

We use a novel cluster identification tool StarGO to explore the metal poor ([Fe/H] -1.5) outer stellar halo (d 15 kpc) of the Milky Way using data from Gaia, LAMOST and SD…

astro-ph.GA2018★ 63 cited

StarGO: A New Method to Identify the Galactic Origins of Halo Stars

Zhen Yuan, Jiang Chang, Projjwal Banerjee +3

We develop a new method StarGO (Stars' Galactic Origin) to identify the galactic origins of halo stars using their kinematics. Our method is based on self-organizing map (SOM), whi…

astro-ph.GA2017★ 38 cited

CALIFA reveals Prolate Rotation in Massive Early-type Galaxies: A Polar Galaxy Merger Origin?

Athanasia Tsatsi, Mariya Lyubenova, Glenn van de Ven +4

We present new evidence for eight early-type galaxies (ETGs) from the CALIFA Survey that show clear rotation around their major photometric axis ("prolate rotation"). These are LSB…

astro-ph.GA2014★ 7 cited

Cold stream stability during minor mergers

Liang Wang, Weishan Zhu, Longlong Feng +3

We use high-resolution Eulerian simulations to study the stability of cold gas flows in a galaxy size dark matter halo (10^12 Msun) at redshift z=2. Our simulations show that a col…