3 citations · 8 across the 4 of their papers we have counts for
7 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…
The origin of the most recently ejected OB runaway star from the R136 cluster
Simon Portegies Zwart, Michel Stoop, Lex Kaper +3
The solar-mass (\MSun) star-cluster R136 (NGC~2070) in the Tarantula Nebula in the Large Magellanic Cloud is the host of at least 55 massive stars ($M \apgt 10$\,\MS…
Why Wide Jupiter-Mass Binary-Objects Cannot Form
Simon Portegies Zwart, Erwan Hochart
The discovery of Jupiter-mass binary objects (JuMBOs) alongside free-floating Jupiter-mass objects (JMOs) in the Trapezium cluster's central por…
Oort Cloud Formation and Evolution in Star Clusters
Justine C. Obidowski, Jeremy J. Webb, Simon Portegies Zwart +1
It is unknown if an Oort cloud reaches its maximum mass within its star's birth cluster or millions of years later. Complicating the Oort cloud evolution process is the fact that c…
Gone with the wind: the impact of wind mass transfer on the orbital evolution of AGB binary systems
M. I. Saladino, O. R. Pols, E. van der Helm +2
In low-mass binary systems, mass transfer is likely to occur via a slow and dense stellar wind when one of the stars is in the AGB phase. Observations show that many binaries that…