activity
19972023
most citedYoung massive star clusters

1.2k citations · 9.9k across the 177 of their papers we have counts for

collaborators
Showing 2014Show all

9 papers · 1 filter

astro-ph.GA2014★ 79 cited

24.77 Pflops on a Gravitational Tree-Code to Simulate the Milky Way Galaxy with 18600 GPUs

Jeroen Bédorf, Evghenii Gaburov, Michiko S. Fujii +3

We have simulated, for the first time, the long term evolution of the Milky Way Galaxy using 51 billion particles on the Swiss Piz Daint supercomputer with our -body gravitation…

astro-ph.CO2014

The cosmic web in CosmoGrid void regions

Steven Rieder, Rien van de Weygaert, Marius Cautun +2

We study the formation and evolution of the cosmic web, using the high-resolution CosmoGrid $Λ$CDM simulation. In particular, we investigate the evolution of the large-scale stru…

astro-ph.IM2014★ 3 cited

Computational Gravitational Dynamics with Modern Numerical Accelerators

Simon Portegies Zwart, Jeroen Bédorf

We review the recent optimizations of gravitational -body kernels for running them on graphics processing units (GPUs), on single hosts and massive parallel platforms. For each…

astro-ph.GA2014★ 10 cited

On the Effects of Subvirial Initial Conditions and the Birth Temperature of R136

Daniel Caputo, Nathan de Vries, Simon Portegies Zwart

We investigate the effect of different initial virial temperatures, Q, on the dynamics of star clusters. We find that the virial temperature has a strong effect on many aspects of…

astro-ph.GA2014★ 40 cited

Star Formation in the vicinity of Nuclear Black Holes: Young Stellar Objects close to Sgr A*

B. Jalali, F. I. Pelupessy, A. Eckart +6

It is often assumed that the strong gravitational field of a super-massive black hole disrupts an adjacent molecular cloud preventing classical star formation in the deep potential…

astro-ph.IM2014★ 15 cited

A connected component-based method for efficiently integrating multiscale -body systems

Jürgen Jänes, Federico I. Pelupessy, Simon F. Portegies Zwart

We present a novel method for efficient direct integration of gravitational N-body systems with a large variation in characteristic time scales. The method is based on a recursive…