activity
20042019
most citedA multiphysics and multiscale software environment for modeling astrophysical systems

201 citations · 323 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR2019★ 30 cited

Evidence from high mass X-ray binaries that Galactic WR components of WR+O binaries end their life with a supernova explosion

D. Vanbeveren, N. Mennekens, E. P. J. van den Heuvel +1

Theoretical population number studies of binaries with at least one black hole (BH) component are obviously depending on whether or not BHs receive a (natal) kick during their form…

cs.DC2019★ 1 cited

Report on energy-efficiency evaluation of several NWP model configurations

Joris Van Bever, Alex McFaden, Zbigniew Piotrowski +1

This document is one of the deliverable reports created for the ESCAPE project. ESCAPE stands for Energy-efficient Scalable Algorithms for Weather Prediction at Exascale. The proje…

astro-ph2008★ 201 cited

A multiphysics and multiscale software environment for modeling astrophysical systems

Simon Portegies Zwart, Steve McMillan, Stefan Harfst +2

We present MUSE, a software framework for combining existing computational tools for different astrophysical domains into a single multiphysics, multiscale application. MUSE facili…

astro-ph2008

Binary populations and stellar dynamics in young clusters

D. Vanbeveren, H. Belkus, J. Van Bever +1

We first summarize work that has been done on the effects of binaries on theoretical population synthesis of stars and stellar phenomena. Next, we highlight the influence of stella…

astro-ph2007

The formation and evolution of very massive stars in dense stellar systems

H. Belkus, J. Van Bever, D. Vanbeveren

The early evolution of dense stellar systems is governed by massive single star and binary evolution. Core collapse of dense massive star clusters can lead to the formation of very…

astro-ph2007★ 91 cited

The WR population predicted by massive single star and by massive binary evolution

D. Vanbeveren, J. Van Bever, H. Belkus

We discuss differences between massive single star and massive close binary population number synthesis predictions of WR stars. We show that the WC/WN number ratio as function of…