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20052023
most citedDynamical Outcomes of Planet-Planet Scattering

932 citations · 8.6k across the 92 of their papers we have counts for

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Showing 2021 · astro-ph.GAShow all

6 papers · 2 filters

astro-ph.GA2021★ 55 cited

Gaia May Detect Hundreds of Well-characterised Stellar Black Holes

Chirag Chawla, Sourav Chatterjee, Katelyn Breivik +3

Detection of black holes (BHs) with detached luminous companions (LCs) can be instrumental in connecting the BH properties with their progenitors' since the latter can be inferred…

astro-ph.GA2021★ 113 cited

Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Monte Carlo Code

Carl L. Rodriguez, Newlin C. Weatherford, Scott C. Coughlin +10

We describe the public release of the Cluster Monte Carlo Code (CMC) a parallel, star-by-star -body code for modeling dense star clusters. CMC treats collisional stellar dynamic…

astro-ph.GA2021★ 57 cited

White Dwarf Subsystems in Core-Collapsed Globular Clusters

Kyle Kremer, Nicholas Z. Rui, Newlin C. Weatherford +5

Numerical and observational evidence suggests that massive white dwarfs dominate the innermost regions of core-collapsed globular clusters by both number and total mass. Using NGC…

astro-ph.GA2021★ 18 cited

No Black Holes in NGC 6397

Nicholas Z. Rui, Newlin Weatherford, Kyle Kremer +5

Recently, \citet{vitral2021does} detected a central concentration of dark objects in the core-collapsed globular cluster NGC 6397, which could be interpreted as a subcluster of ste…

astro-ph.GA2021★ 26 cited

Matching Globular Cluster Models to Observations

Nicholas Z. Rui, Kyle Kremer, Newlin C. Weatherford +4

As ancient, gravitationally bound stellar populations, globular clusters are abundant, vibrant laboratories characterized by high frequencies of dynamical interactions coupled to c…

astro-ph.GA2021★ 46 cited

Black Hole Mergers from Star Clusters with Top-Heavy Initial Mass Functions

Newlin C. Weatherford, Giacomo Fragione, Kyle Kremer +4

Recent observations of globular clusters (GCs) provide evidence that the stellar initial mass function (IMF) may not be universal, suggesting specifically that the IMF grows increa…