activity
20032025
most citedA Dynamical Model for the Globular Cluster G1

166 citations · 234 across the 6 of their papers we have counts for

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Showing 2025Show all

5 papers · 1 filter

astro-ph.GA2025

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…

astro-ph.GA2025

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…

astro-ph.SR2025★ 2 cited

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…

astro-ph.EP2025★ 3 cited

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…

astro-ph.EP2025★ 3 cited

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…