activity
19932026
most citedDynamical Outcomes of Planet-Planet Scattering

932 citations · 21.6k across the 237 of their papers we have counts for

collaborators
Showing astro-ph.SRShow all

16 papers · 1 filter

astro-ph.SR2026

Using Machine Learning to Model Stellar Collisions in our Galactic Center

Tristan C. Sand, Sanaea C. Rose, Elena González Prieto +8

Direct collisions in the inner pc of the Galactic center can alter the orbits and properties of stars. The outcome of a collision depends on a number of parameters, including the m…

astro-ph.SR2024

Formation of Stripped Stars From Stellar Collisions in Galactic Nuclei

C. Gibson, F. Kıroğlu, J. C. Lombardi +7

Tidal disruption events (TDEs) are an important way to probe the properties of stellar populations surrounding supermassive black holes. Observed spectra of several TDEs, such as A…

astro-ph.SR2024

Can slow pulsars in Milky Way globular clusters form via partial recycling?

Kyle Kremer, Claire S. Ye, Craig O. Heinke +3

Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods $0.3-4\,…

astro-ph.SR2024★ 1 cited

On Binary Formation from Three Initially Unbound Bodies

Dany Atallah, Newlin C. Weatherford, Alessandro A. Trani +1

We explore three-body binary formation (3BBF), the formation of a bound system via gravitational scattering of three initially unbound bodies (3UB), using direct numerical integrat…

astro-ph.SR2019★ 77 cited

A Dynamical Survey of Stellar-Mass Black Holes in 50 Milky Way Globular Clusters

Newlin C. Weatherford, Sourav Chatterjee, Kyle Kremer +1

Recent numerical simulations of globular clusters (GCs) have shown that stellar-mass black holes (BHs) play a fundamental role in driving cluster evolution and shaping their presen…

astro-ph.SR2019★ 50 cited

In Search of the Thermal Eccentricity Distribution

Aaron M. Geller, Nathan W. C. Leigh, Mirek Giersz +2

About a century ago, Jeans (1919) discovered that if binary stars reach a state approximating energy equipartition, for example through many dynamical encounters that exchange ener…