activity
20152021
most citedBarred Galaxies in the IllustrisTNG Simulation

57 citations · 343 across the 11 of their papers we have counts for

collaborators

11 papers

astro-ph.GA2021★ 34 cited

The Diverse Morphology, Stellar Population, and Black Hole Scaling Relations of the Host Galaxies of Nearby Quasars

Yulin Zhao, Luis C. Ho, Jinyi Shangguan +3

We present rest-frame and imaging of 35 low-redshift () Palomar-Green quasars using the Hubble Space Telescope Wide Field Camera 3. We perform multi-component two-…

astro-ph.GA2020★ 57 cited

Barred Galaxies in the IllustrisTNG Simulation

Dongyao Zhao, Min Du, Luis C. Ho +2

Almost two-thirds of disk galaxies in the local universe host bars, which serve as important drivers of secular evolutionary processes. While cosmological simulations are powerful…

astro-ph.CO2020★ 19 cited

Orbital distribution of infalling satellite halos across cosmic time

Zhao-Zhou Li, Dong-Hai Zhao, Y. P. Jing +2

The initial orbits of infalling subhalos largely determine the subsequent evolution of the subhalos and satellite galaxies therein and shed light on the assembly of their hosts. Us…

astro-ph.GA2020★ 48 cited

Kinematic decomposition of IllustrisTNG disk galaxies: morphology and relation with morphological structures

Min Du, Luis C. Ho, Victor P. Debattista +4

We recently developed an automated method, auto-GMM to decompose simulated galaxies. It extracts kinematic structures in an accurate, efficient, and unsupervised way. We use auto-G…

astro-ph.GA2019★ 17 cited

A New Channel of Bulge Formation via The Destruction of Short Bars

Minghao Guo, Min Du, Luis C. Ho +2

Short (inner) bars of sub-kiloparsec radius have been hypothesized to be an important mechanism for driving gas inflows to small scales, thus feeding central black holes. Recent nu…

astro-ph.GA2019★ 43 cited

Identifying kinematic structures in simulated galaxies using unsupervised machine learning

Min Du, Luis C. Ho, Dongyao Zhao +4

Galaxies host a wide array of internal stellar components, which need to be decomposed accurately in order to understand their formation and evolution. While significant progress h…

astro-ph.GA2019★ 32 cited

The Role of Major Mergers and Nuclear Star Formation in Nearby Obscured Quasars

Dongyao Zhao, Luis C. Ho, Yulin Zhao +2

We investigate the triggering mechanism and the structural properties of obscured luminous active galactic nuclei from a detailed study of the rest-frame and HST images of…

astro-ph.GA2017★ 25 cited

Determination of Dark Matter Halo Mass from Dynamics of Satellite Galaxies

Zhao-Zhou Li, Y. P. Jing, Yong-Zhong Qian +2

We show that the mass of a dark matter halo can be inferred from the dynamical status of its satellite galaxies. Using 9 dark-matter simulations of halos like the Milky Way (MW), w…

astro-ph.GA2016★ 16 cited

Exploring the progenitors of brightest cluster galaxies at z~2

Dongyao Zhao, Christopher J. Conselice, Alfonso Aragón-Salamanca +5

We present a new method for tracing the evolution of BCGs from to . We conclude on the basis of semi-analytical models that the best method to select BCG progeni…

astro-ph.GA2015★ 32 cited

Evolution of the brightest cluster galaxies: the influence of morphology, stellar mass and environment

Dongyao Zhao, Alfonso Aragón-Salamanca, Christopher J. Conselice

Using a sample of 425 nearby Brightest Cluster Galaxies (BCGs) from von der Linden et al. (2007), we study the relationship between their internal properties (stellar masses, struc…

astro-ph.GA2015★ 20 cited

The Link Between Morphology and Structure of Brightest Cluster Galaxies: Automatic Identification of cDs

Dongyao Zhao, Alfonso Aragón-Salamanca, Christopher J. Conselice

We study a large sample of 625 low-redshift brightest cluster galaxies (BCGs) and link their morphologies to their structural properties. We derive visual morphologies and find tha…