activity
19942022
most citedSpatial correlation function and pairwise velocity dispersion of galaxies: CDM models versus the Las Campanas Survey

434 citations · 1.3k across the 18 of their papers we have counts for

collaborators

18 papers

astro-ph.GA2022★ 1 cited

Shock-induced stripping of satellite ISM/CGM in IllustrisTNG clusters at

Hao Li, Huiyuan Wang, H. J. Mo +3

Using the IllustrisTNG simulation, we study the interaction of large-scale shocks with the circumgalactic medium (CGM) and interstellar medium (ISM) of star-forming (SF) satellite…

astro-ph.CO2021★ 5 cited

Evaluating the origins of the secondary bias based on the correlation of halo properties with the linear density field

Xiaoyu Wang, Huiyuan Wang, H. J. Mo +2

Using two sets of large -body simulations, we study the origin of the correlations of halo assembly time (), concentration () and spin ()…

astro-ph.IM2021★ 31 cited

HUBS: A dedicated hot circumgalactic medium explorer

Wei Cui

The Hot Universe Baryon Surveyor (HUBS) mission is proposed to study "missing" baryons in the universe. Unlike dark matter, baryonic matter is made of elements in the periodic tabl…

astro-ph.GA2017★ 75 cited

ELUCID IV: Galaxy Quenching and its Relation to Halo Mass, Environment, and Assembly Bias

Huiyuan Wang, H. J. Mo, Sihan Chen +17

We examine the quenched fraction of central and satellite galaxies as a function of galaxy stellar mass, halo mass, and the matter density of their large scale environment. Matter…

astro-ph.CO2016★ 142 cited

ELUCID - Exploring the Local Universe with reConstructed Initial Density field III: Constrained Simulation in the SDSS Volume

Huiyuan Wang, H. J. Mo, Xiaohu Yang +7

A method we developed recently for the reconstruction of the initial density field in the nearby Universe is applied to the Sloan Digital Sky Survey Data Release 7. A high-resoluti…

astro-ph.GA2015

Star Formation and Quenching of Satellite Galaxies

Zhankui Lu, H. J. Mo

We study the quenching of satellite galaxies by gradual depletion of gas due to star formation, by ram-pressure striping and by tidally triggered starburst. Using progenitors const…