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20142026
most citedBarred galaxies in the Illustris-1 and TNG100 simulations

44 citations · 239 across the 30 of their papers we have counts for

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Showing astro-ph.GAShow all

11 papers · 1 filter

astro-ph.GA2026

Properties of Galactic Outflows Driven by Starburst at Cosmic Noon: Insights from Hydrodynamical Simulations

Huan Chen, Weishan Zhu, Xue-Fu Li +3

We investigate starburst-driven galactic outflows in low-mass galaxies () at cosmic noon using high-resolution 3D hydrodynamical simulations based o…

astro-ph.GA2025★ 1 cited

Gamma Analytical Modeling Evolution (GAME) I: The physical implications of deriving the stellar mass functions from z=0 to z=8

Antonios Katsianis, Qingshan Wang, Xiaohu Yang +13

The growth model is an effective parameterization employed across various scientific disciplines and scales to depict growth. It has been demonstrated that the cosmic star form…

astro-ph.GA2025★ 4 cited

Impact of cosmic web on the properties of galaxies in IllustrisTNG simulations

Guangyao Yu, Weishan Zhu, Qi-Rui Yang +3

We investigate the influence of the cosmic web on galaxy properties in the IllustrisTNG simulations. To disentangle the effects of galaxy groups and cosmic filaments, we classify t…

astro-ph.GA2024

Revisiting the Galactic Winds in M82 I: the recent starburst and launch of outflow in simulations

Tian-Rui Wang, Weishan Zhu, Xue-Fu Li +2

We revisit the launch of the galactic outflow in M82 using hydrodynamic simulations. Employing a sink-particle module, we self-consistently resolve star formation and feedback, avo…

astro-ph.GA2024★ 3 cited

Revisiting the Galactic Winds in M82 II: Development of Multiphase Outflows in Simulations

Xue-Fu Li, Weishan Zhu, Tian-Rui Wang +1

We performed a suit of three-dimensional hydrodynamical simulations with a resolution of parsecs to investigate the development of multiphase galactic wind in M82. The sta…

astro-ph.GA2024★ 4 cited

Evolution of cold streams in hot gaseous halos

WenSheng Hong, Weishan Zhu, TianRui Wang +2

In the prevailing model of galaxy formation and evolution, the process of gas accretion onto central galaxies undergoes a transition from cold-dominated to hot-dominated modes. Thi…

astro-ph.GA2021★ 14 cited

Impact of cosmic filaments on the gas accretion rate of dark matter halos

Weishan Zhu, Fupeng Zhang, Long-Long Feng

We investigate the impact of cosmic filaments on the gas accretion rate, , of dark matter halos in filaments, based on cosmological hydrodynamic simulation. We…

astro-ph.GA2020★ 44 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★ 3 cited

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…

astro-ph.GA2017★ 2 cited

Pre-heating of the intergalactic medium by gravitational collapse and ultraviolet background

Weishan Zhu, Long-Long Feng

The preheating of intergalactic medium(IGM) by structure collapsing and ultraviolet background(UVB) are investigated in cosmological hydrodynamical simulations. When gravitational…

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…