1.2k citations · 1.6k across the 11 of their papers we have counts for
12 papers
Transferring Data from a Voronoi Mesh to an Adaptive Cartesian Grid in Pursuit of Self-consistent Top-down Star Formation
Sean C. Lewis, Brooke Polak, Mordecai-Mark Mac Low +5
Unstructured Voronoi mesh simulations offer many advantages for simulating self-gravitating gas dynamics on galactic scales. Adaptive mesh refinement (AMR) can be a powerful tool f…
Protostellar Jets in Star Cluster Formation and Evolution: I. Implementation and Initial Results
Sabrina M. Appel, Blakesley Burkhart, Mordecai-Mark Mac Low +8
Stars form in clusters from the gravitational collapse of giant molecular clouds, which is opposed by a variety of physical processes, including stellar feedback. The interplay bet…
Massive Star Cluster Formation with Binaries. I. Evolution of Binary Populations
Claude Cournoyer-Cloutier, Alison Sills, William E. Harris +7
We study the evolution of populations of binary stars within massive cluster-forming regions. We simulate the formation of young massive star clusters within giant molecular clouds…
Massive star cluster formation III. Early mass segregation during cluster assembly
Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +6
Mass segregation is seen in many star clusters, but whether massive stars form in the center of a cluster or migrate there dynamically is still debated. N-body simulations have sho…
Massive star cluster formation II. Runaway stars as fossils of sub-cluster mergers
Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +6
Two main mechanisms have classically been proposed for the formation of runaway stars. In the binary supernova scenario (BSS), a massive star in a binary explodes as a supernova, e…
Massive star cluster formation I. High star formation efficiency while resolving feedback of individual stars
Brooke Polak, Mordecai-Mark Mac Low, Ralf S. Klessen +11
The mode of star formation that results in the formation of globular clusters and young massive clusters is difficult to constrain through observations. We present models of massiv…
Multi-physics simulations using a hierarchical interchangeable software interface
Simon Portegies Zwart, Steve McMillan, Arjen van Elteren +2
We introduce a general-purpose framework for interconnecting scientific simulation programs using a homogeneous, unified interface. Our framework is intrinsically parallel, and con…
Multi-physics simulations using a hierarchical interchangeable software interface
Simon Portegies Zwart, Stephen McMillan, Inti Pelupessy +1
We introduce a general-purpose framework for interconnecting scientific simulation programs using a homogeneous, unified software interface. Our framework is intrinsically parallel…
Young massive star clusters
Simon Portegies Zwart, Steve McMillan, Mark Gieles
Young massive clusters are dense aggregates of young stars that form the fundamental building blocks of galaxies. Several examples exist in the Milky Way Galaxy and the Local Group…
Simulating the universe on an intercontinental grid of supercomputers
Simon Portegies Zwart, Tomoaki Ishiyama, Derek Groen +7
Understanding the universe is hampered by the elusiveness of its most common constituent, cold dark matter. Almost impossible to observe, dark matter can be studied effectively by…
Binary--single-star scattering VII. Hard Binary Exchange Cross Sections for Arbitrary Mass Ratios: Numerical Results and Semi-Analytic Fits
D. C. Heggie, P. Hut, S. L. W. McMillan
We present the first comprehensive fitting formula for exchange reactions of arbitrary mass ratios. In a comparison with numerical results, this expression is shown to be accurate…
Gravitational Radiation from Coalescing Binary Neutron Stars
Xing Zhuge, Joan M. Centrella, Stephen L. W. McMillan
We calculate the gravitational radiation produced by the merger and coalescence of inspiraling binary neutron stars using 3-dimensional numerical simulations. The stars are modeled…