activity
20172023
most citedA Three-Dimensional View of Turbulence: Constraints on Turbulent Motions in the HD 163296 Protoplanetary Disk using DCO

286 citations · 355 across the 4 of their papers we have counts for

collaborators

6 papers

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.GA2023

Tidal Disruption Events from the Combined Effects of Two-Body Relaxation and the Eccentric Kozai-Lidov Mechanism

Denyz Melchor, Brenna Mockler, Smadar Naoz +2

Tidal disruption events (TDEs) take place when a star ventures too close to a supermassive black hole (SMBH) and becomes ruptured. One of the leading proposed physical mechanisms o…

astro-ph.HE202245 cited

The Combined Effects of Two-Body Relaxation Processes and the Eccentric Kozai-Lidov Mechanism on the EMRI Rate

Smadar Naoz, Sanaea C. Rose, Erez Michaely +4

Gravitational wave (GW) emissions from extreme-mass-ratio inspirals (EMRIs) are promising sources for low-frequency GW-detectors. They result from a compact object, such as a stell…

astro-ph.SR2020

On Socially Distant Neighbors: Using Binaries to Constrain the Density of Objects in the Galactic Center

Sanaea C. Rose, Smadar Naoz, Abhimat K. Gautam +4

Stars often reside in binary configurations. The nuclear star cluster surrounding the supermassive black hole (SMBH) in the Galactic Center (GC) is expected to include a binary pop…

astro-ph.SR201924 cited

Companion-driven evolution of massive stellar binaries

Sanaea C. Rose, Smadar Naoz, Aaron M. Geller

At least of massive OBA-type stars reside in binary or higher-order systems. The dynamical evolution of these systems can lend insight into the origins of extreme phenomena…

astro-ph.EP2017286 cited

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

Kevin M. Flaherty, A. Meredith Hughes, Sanaea C. Rose +8

Gas kinematics are an important part of the planet formation process. Turbulence influences planetesimal growth and migration from the scale of sub-micron dust grains through gas-g…