activity
20112024
most citedThe stellar mass assembly of galaxies in the Illustris simulation: growth by mergers and the spatial distribution of accreted stars

478 citations · 1.2k across the 27 of their papers we have counts for

collaborators

27 papers

astro-ph.GA2024

Environmental effects on Low Surface Brightness Galaxies in the IllustrisTNG simulation

Luis Enrique Pérez-Montaño, Bernardo Cervantes Sodi, Vicente Rodriguez-Gomez +2

Employing the TNG100 run of the IllustrisTNG project, we characterize the environment of Low Surface Brightness Galaxies (LSBGs) across varying scales, from their associated dark m…

astro-ph.GA2022★ 33 cited

The formation of low surface brightness galaxies in the IllustrisTNG simulation

Luis Enrique Pérez-Montaño, Vicente Rodriguez-Gomez, Bernardo Cervantes Sodi +4

We explore the nature of low surface brightness galaxies (LSBGs) in the hydrodynamic cosmological simulation TNG100 of the IllustrisTNG project, selecting a sample of LSBGs (-ba…

astro-ph.GA2022★ 9 cited

Evolution of Massive Black Hole Binaries in Collisionally Relaxed Nuclear Star Clusters -- Impact of Mass Segregation

Diptajyoti Mukherjee, Qirong Zhu, Go Ogiya +2

Massive Black Hole (MBH) binaries are considered to be one of the most important sources of Gravitational Waves (GW) that can be detected by GW detectors like LISA. However, there…

astro-ph.GA2020★ 18 cited

The Formation of the First Quasars. I. The Black Hole Seeds, Accretion and Feedback Models

Qirong Zhu, Yuexing Li, Yiting Li +4

Supermassive black holes (SMBHs) of are generally believed to be the central engines of the luminous quasars observed at , but their astrophysical…

astro-ph.GA2020★ 13 cited

Fast Multipole Methods for -body Simulations of Collisional Star Systems

Diptajyoti Mukherjee, Qirong Zhu, Hy Trac +1

Direct -body simulations of star clusters are accurate but expensive, largely due to the numerous pairwise force calculations. To solve the post-million-body…

astro-ph.GA2020★ 16 cited

ART: A 3D Parallel Multi-wavelength Radiative Transfer Code for Continuum and Atomic and Molecular Lines

Yuexing Li, Ming F. Gu, Hidenobu Yajima +2

ART is a 3D multi-wavelength Monte Carlo radiative transfer (RT) code that couples continuum and emission lines to track the propagation of photons and their interactions with…