76 citations · 246 across the 7 of their papers we have counts for
7 papers
A Monte Carlo study of early gas expulsion and evolution of star clusters: new simulations with the MOCCA code in the AMUSE framework
A. Leveque, M. Giersz, S. Banerjee +3
We introduce a new prescription for the evolution of globular clusters (GCs) during the initial embedded gas phase into a Monte Carlo method. With a simplified version of the Monte…
Survey of Orion Disks with ALMA (SODA) I: Cloud-level demographics of 873 protoplanetary disks
S. E. van Terwisga, A. Hacar, E. F. van Dishoeck +2
(Abridged) Surveys of protoplanetary disks in nearby star-forming regions (SFRs) have provided important information on their demographics, but due to their sample sizes, they cann…
Stellar triples on the edge; Comprehensive overview of the evolution of destabilised triples leading to stellar and binary exotica
S. Toonen, T. C. N. Boekholt, S. Portegies Zwart
Hierarchical triple stars are ideal laboratories for studying the interplay between orbital dynamics and stellar evolution. Both stellar wind mass loss and three-body dynamics coop…
Asymmetric supernova in hierarchical multiple star systems and application to J1903+0327
J. T. Pijloo, D. P. Caputo, S. F. Portegies Zwart
We develop a method to analyze the effect of an asymmetric supernova on hierarchical multiple star systems and we present analytical formulas to calculate orbital parameters for su…
How well do STARLAB and NBODY compare? II: Hardware and accuracy
P. Anders, H. Baumgardt, E. Gaburov +1
Most recent progress in understanding the dynamical evolution of star clusters relies on direct N-body simulations. Owing to the computational demands, and the desire to model more…
The formation of the eccentric-orbit millisecond pulsar J1903+0327 and the origin of single millisecond pulsars
Simon Portegies Zwart, Ed van den Heuvel, Joeri van Leeuwen +1
The millisecond pulsar J1903+0327 is accompanied by an ordinary G-dwarf star in an unusually wide (\,days) and eccentric () orbit. The stand…