activity
20072009
most citedA multiphysics and multiscale software environment for modeling astrophysical systems

201 citations · 529 across the 7 of their papers we have counts for

collaborators

7 papers

astro-ph.SR20094 cited

On the Dynamical Evolution of the Arches Cluster

Sourav Chatterjee, Sanghamitra Goswami, Stefan Umbreit +3

We study the dynamical evolution of the young star cluster Arches and its dependence on the assumed initial stellar mass function (IMF). We perform many direct -body simulations…

astro-ph2008109 cited

Thermohaline mixing and gravitational settling in carbon-enhanced metal-poor stars

Richard J. Stancliffe, Evert Glebbeek

We investigate the formation of carbon-enhanced metal-poor (CEMP) stars via the scenario of mass transfer from a carbon-rich asymptotic giant branch (AGB) primary to a low-mass com…

astro-ph2008201 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-ph200852 cited

Evolution of stellar collision products in open clusters. II. A grid of low-mass collisions

E. Glebbeek, O. R. Pols

In a companion paper we studied the detailed evolution of stellar collision products that occurred in an -body simulation of the old open cluster M67 and compared our detailed m…

astro-ph200867 cited

Evolution of stellar collision products in open clusters. I. Blue stragglers in N-body models of M67

E. Glebbeek, O. R. Pols, J. R. Hurley

Stellar collisions are an important formation channel for blue straggler stars in globular and old open clusters. Hydrodynamical simulations have shown that the remnants of such co…

astro-ph200796 cited

Orbital eccentricities of binary systems with a former AGB star

A. A. Bonacic Marinovic, E. Glebbeek, O. R. Pols

Many binary stellar systems in which the primary star is beyond the asymptotic giant branch (AGB) evolutionary phase show significant orbital eccentricities whereas current binary…