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20172026
most citedA Three-Dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk using DCO

286 citations · 488 across the 20 of their papers we have counts for

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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.GA2026

A cosmological framework for stellar collisions at high redshift in proto-globular clusters, nuclear star clusters, and Little Red Dots

Claire E. Williams, Smadar Naoz, Sanaea C. Rose +8

Observations and cosmological simulations indicate that the early Universe hosted numerous compact, high-density stellar systems, where close encounters and physical collisions bet…

astro-ph.GA2026

IRS 9: The Case for a Dynamically-Ejected Star from the Galactic Center

Matthew Hosek, Tuan Do, Smadar Naoz +7

Measuring stellar motions at the Milky Way's Galactic center (GC) provides unique insight into the dynamical processes within galactic nuclei. We present proper motion measurements…

astro-ph.HE2026

Machine Learning Methods for Stellar Collisions. I. Predicting Outcomes of SPH Simulations

Elena González Prieto, James C. Lombardi, Sanaea C. Rose +7

Stellar collisions can occur frequently in dense cluster environments, and play a crucial role in producing exotic phenomena from blue stragglers in globular clusters to high-energ…

astro-ph.GA2026

Intermediate-Mass Black Hole Formation from Hierarchical Mergers in Galactic Nuclei

Amanda Newton, Sanaea C. Rose, Fulya Kıroğlu +2

Dense stellar environments like nuclear star clusters (NSCs) can dynamically assemble gravitational wave (GW) sources. We consider a population of single stellar mass black holes (…