activity
20132021
most citedThe dynamics of stellar disks in live dark-matter halos

66 citations · 177 across the 5 of their papers we have counts for

collaborators

6 papers

astro-ph.GA2021★ 11 cited

Impact of bar resonances in the velocity-space distribution of the solar neighbourhood stars in a self-consistent -body Galactic disc simulation

Tetsuro Asano, Michiko S. Fujii, Junichi Baba +3

The velocity-space distribution of the solar neighbourhood stars shows complex substructures. Most of the previous studies use static potentials to investigate their origins. Inste…

astro-ph.IM2020★ 7 cited

DeepGalaxy: Deducing the Properties of Galaxy Mergers from Images Using Deep Neural Networks

Maxwell X. Cai, Jeroen Bédorf, Vikram A. Saletore +4

Galaxy mergers, the dynamical process during which two galaxies collide, are among the most spectacular phenomena in the Universe. During this process, the two colliding galaxies a…

astro-ph.IM2019

Bonsai-SPH: A GPU accelerated astrophysical Smoothed Particle Hydrodynamics code

Jeroen Bédorf, Simon Portegies Zwart

We present the smoothed-particle hydrodynamics simulation code, Bonsai-SPH, which is a continuation of our previously developed gravity-only hierarchical -body code (called Bons…

astro-ph.GA2018★ 52 cited

Modeling the Milky Way as a Dry Galaxy

Michiko S. Fujii, Jeroen Bédorf, Junichi Baba +1

We construct a model for the Milky Way Galaxy composed of a stellar disc and bulge embedded in a dark-matter halo. All components are modelled as -body systems with up to 8 bill…

astro-ph.GA2017★ 66 cited

The dynamics of stellar disks in live dark-matter halos

Michiko S. Fujii, Jeroen Bédorf, Junichi Baba +1

Recent developments in computer hardware and software enable researchers to simulate the self-gravitating evolution of galaxies at a resolution comparable to the actual number of s…

astro-ph.GA2013★ 41 cited

The Effect of Many Minor Mergers on the Size Growth of Compact Quiescent Galaxies

Jeroen Bédorf, Simon Portegies Zwart

Massive galaxies with a half-mass radius <~ 1kpc are observed in the early universe (z~>2), but not in the local universe. In the local universe similar-mass (within a factor of tw…