activity
20082026
most citedOrbital decomposition of CALIFA spiral galaxies

105 citations · 1.3k across the 44 of their papers we have counts for

collaborators

44 papers

astro-ph.GA2026

The GECKOS survey: Assembly history of the lenticular galaxy NGC 3957

Yuchen Ding, Marie Martig, Ling Zhu +24

We analyse the assembly history of the edge-on lenticular galaxy NGC 3957 using deep integral-field spectroscopic MUSE data from the GECKOS survey. By applying a dust-corrected Mul…

astro-ph.GA2026

Dissecting the 3D chemo-dynamical structures of NGC~1381: A galaxy hosting an ancient slow bar with an accretion-related bulge and thick disc

Yunpeng Jin, Ling Zhu, Shude Mao +4

We applied the barred population-orbit superposition method developed in our 2025 papers to construct 3D chemo-dynamical models for the barred S0 galaxy NGC~1381 in the Fornax clus…

astro-ph.GA2024

Dark matter measurements combining stellar and HI kinematics: 30% outliers with low dark matter content at

Meng Yang, Ling Zhu, Yu Lei +5

We construct the Schwarzschild dynamical models for 11 early-type galaxies with the SAURON and Mitchell stellar IFUs out to , and construct dynamical models with…

astro-ph.GA2024

Uncovering the formation of the counter-rotating stellar disks in SDSS J074834.64+444117.8

Min Bao, Yanmei Chen, Meng Yang +3

Using the integral field spectroscopic data from Mapping Nearby Galaxies at Apache Point Observatory survey, we study the kinematics and stellar population properties of the two co…

astro-ph.GA2024

The internal dynamics and environments of Relics and compact massive ETGs with TNG50

Micheli T. Moura, Ana L. Chies-Santos, Cristina Furlanetto +2

Relic galaxies are massive, compact, quiescent objects observed in the local Universe that have not experienced any significant interaction episodes or merger events since about $z…

astro-ph.GA2023

Unraveling the Complexity of Dwarf Galaxy Dynamics: A study of Binary Orbital Motions

Wenting Wang, Ling Zhu, Yipeng Jing +8

We investigate the impact of binary orbital motions on the dynamical modeling of dwarf galaxies with intrinsic line-of-sight velocity dispersions () of 1 to 9 km/s. Using…

astro-ph.GA2022★ 15 cited

Constructing the Milky Way Stellar Halo in the Galactic Center by Direct Orbit Integration

Chengqun Yang, Ling Zhu, Behzad Tahmasebzadeh +2

The halo stars on highly radial orbits should inevitably pass the center regions of the Milky Way. Under the assumption that the stellar halo is in dynamical equilibrium and axisym…

astro-ph.GA2022★ 21 cited

Orbit-Superposition Dynamical Modeling of Barred Galaxies

Behzad Tahmasebzadeh, Ling Zhu, Juntai Shen +2

Barred structures are important in understanding galaxy evolution, but they were not included explicitly in most dynamical models for nearby galaxies due to their complicated morph…

astro-ph.GA2022★ 42 cited

Milky Way Mass with K Giants and BHB Stars Using LAMOST, SDSS/SEGUE, and Gaia: 3D Spherical Jeans Equation and Tracer Mass Estimator

Sarah A. Bird, Xiang-Xiang Xue, Chao Liu +8

We measure the enclosed Milky Way mass profile to Galactocentric distances of and kpc using the smooth, diffuse stellar halo samples of Bird et al. The samples ar…

astro-ph.GA2022★ 11 cited

Is the core-cusp problem a matter of perspective: Jeans Anisotropic Modeling against numerical simulations

Wenting Wang, Ling Zhu, Zhaozhou Li +14

Mock member stars for 28 dwarf galaxies are constructed from the cosmological Auriga simulation, which reflect the dynamical status of realistic stellar tracers. The axis-symmetric…

astro-ph.GA2022★ 32 cited

The Fornax3D project: discovery of ancient massive merger events in the Fornax cluster galaxies NGC 1380 and NGC 1427

Ling Zhu, Glenn van de Ven, Ryan Leaman +16

We report the discovery of ancient massive merger events in the early-type galaxies NGC 1380 and NGC 1427, members of the Fornax galaxy cluster. Both galaxies have been observed by…

astro-ph.GA2022★ 52 cited

The SAMI Galaxy Survey: The internal orbital structure and mass distribution of passive galaxies from triaxial orbit-superposition Schwarzschild models

Giulia Santucci, Sarah Brough, Jesse van de Sande +17

Dynamical models are crucial for uncovering the internal dynamics of galaxies, however, most of the results to date assume axisymmetry, which is not representative for a significan…

astro-ph.GA2022★ 15 cited

Different Formation Scenarios of Counter-rotating Stellar Disks in Nearby Galaxies

Min Bao, Yanmei Chen, Pengpei Zhu +7

Using the integral field unit (IFU) data from Mapping Nearby Galaxies at Apache Point Observatory (MaNGA) survey, we select a sample of 101 galaxies with counter-rotating stellar d…

astro-ph.GA2021

Deprojection of external barred galaxies from photometry

Behzad Tahmasebzadeh, Ling Zhu, Juntai Shen +2

The observations of external galaxies are projected to the 2D sky plane. Reconstructing the 3D intrinsic density distribution of a galaxy from the 2D image is challenging, especial…

astro-ph.GA2021★ 39 cited

Mass of the dynamically hot inner stellar halo predicts the ancient accreted stellar mass

Ling Zhu, Annalisa Pillepich, Glenn van de Ven +6

Galactic dynamical structures are fossil records of the assembly histories of galaxies. By analyzing the cosmological hydrodynamical simulation TNG50, we find that a dynamical stru…

astro-ph.GA2020★ 23 cited

Hot and counter-rotating star-forming disk galaxies in IllustrisTNG and their real-world counterparts

Shengdong Lu, Dandan Xu, Yunchong Wang +7

A key feature of a large population of low-mass, late-type disk galaxies are star-forming disks with exponential light distributions. They are typically also associated with thin a…

astro-ph.GA2020★ 16 cited

A discrete chemo-dynamical model of M87's globular clusters: Kinematics extending to ~ 400 kpc

Chao Li, Ling Zhu, R. J. Long +14

We study the mass distribution and kinematics of the giant elliptical galaxy M87 (NGC 4486) using discrete chemo-dynamical, axisymmetric Jeans equation modelling. Our catalogue com…

astro-ph.GA2020★ 3 cited

A Universal fundamental plane and the relation for galaxies with CALIFA and MaNGA

E. Aquino-Ortíz, S. F. Sánchez, O. Valenzuela +8

We use the stellar kinematics for galaxies from the MaNGA survey to explore dynamical scaling relations between the stellar mass and the total velocity parameter…

astro-ph.GA2020★ 9 cited

Unravelling stellar populations in the Andromeda Galaxy

Grzegorz Gajda, Ortwin Gerhard, Matías Blaña +4

To understand the history and formation mechanisms of galaxies it is crucial to determine their current multidimensional structure. Here we focus on stellar population properties,…

astro-ph.GA2020★ 44 cited

Disentangling the formation history of galaxies via population-orbit superposition: method validation

Ling Zhu, Glenn van de Ven, Ryan Leaman +9

We present population-orbit superposition models for external galaxies based on Schwarzschild's orbit-superposition method, by tagging the orbits with age and metallicity. The mode…

astro-ph.GA2019★ 28 cited

SDSS-IV MaNGA: Internal mass distributions and orbital structures of early-type galaxies and their dependence on environment

Yunpeng Jin, Ling Zhu, R. J. Long +3

In our earlier 2019 paper, we evaluated the reliability of Schwarzschild's orbit-superposition dynamical modelling method in estimating the internal mass distribution, intrinsic st…

astro-ph.GA2019★ 15 cited

Mapping the dark matter halo of early-type galaxy NGC 2974 through orbit-based models with combined stellar and cold gas kinematics

Meng Yang, Ling Zhu, Anne-Marie Weijmans +4

We present an orbit-based method of combining stellar and cold gas kinematics to constrain the dark matter profile of early-type galaxies. We apply this method to early-type galaxy…

astro-ph.GA2019★ 6 cited

NGC 7457: Evidence for merger-driven cylindrical rotation in disc galaxies

Alireza Molaeinezhad, Ling Zhu, Jesús Falcón-Barroso +7

We construct Schwarzschild orbit-based models of NGC 7457, known as a peculiar low-mass lenticular galaxy. Our best-fitting model successfully retrieves most of the unusual kinemat…

astro-ph.GA2019★ 39 cited

Constraining nuclear star cluster formation using MUSE-AO observations of the early-type galaxy FCC47

Katja Fahrion, Mariya Lyubenova, Glenn van de Ven +12

Nuclear star clusters (NSCs) are found in at least 70% of all galaxies, but their formation path is still unclear. In the most common scenarios, NSCs form in-situ from the galaxy's…