activity
20172022
most citedBarred galaxies in the Illustris-1 and TNG100 simulations

44 citations · 116 across the 7 of their papers we have counts for

collaborators

10 papers

astro-ph.CO2021

Profiles of cosmic filaments since z=4.0 in cosmological hydrodynamical simulation

Weishan Zhu, Fupeng Zhang, Long-Long Feng

A large portion of the baryons at low redshifts are still missing from detection. Most of the missing baryons are believed to reside in large scale cosmic filaments. Understanding…

astro-ph.GA20205 cited

Estimation of the Galaxy Quenching Rate in the Illustris Simulation

Yang Wang, Xuan Liu, Weishan Zhu +2

Quenching is a key topic in exploring the formation and evolution of galaxies. In this work, we study the quenching rate, i.e., the variation in the fraction of quenched galaxies p…

astro-ph.HE202029 cited

The dispersion measure and scattering of FRBs: Contributions from the intergalactic medium, foreground halos, and hosts

Weishan Zhu, Long-Long Feng

We investigate the dispersion measure(DM) and scattering of FRBs by the intergalactic-medium(IGM), foreground and host halos, using cosmological hydrodynamical simulation. We find…

astro-ph.CO20207 cited

Turbulence-induced deviation between baryonic field and dark matter field in the spatial distribution of the Universe

Hua-Yu Yang, Ping He, Weishan Zhu +1

The cosmic baryonic fluid at low redshifts is similar to a fully developed turbulence. In this work, we use simulation samples produced by the hybrid cosmological hydrodynamical/N-…

astro-ph.GA202044 cited

Barred galaxies in the Illustris-1 and TNG100 simulations

Ze-Bang Zhou, Weishan Zhu, Yang Wang +1

We carry out a comparison study on the bar structure in the Illustris-1 and TNG100 simulations. At , 8.9\% of 1232 disc galaxies with stellar mass in Ill…

astro-ph.GA2020

The temperature of IGM at high redshifts: shock heating and high mach problem

Junyi Jia, Weishan Zhu, Liang Gao +1

The thermal history of cosmic gas in the Dark Ages remains largely unknown. It is important to quantify the impact of relevant physics on the IGM temperature between and $z…