output
19972023
most citedA multiphysics and multiscale software environment for modeling astrophysical systems

201 citations

35 papers

astro-ph.HE2023★ 15 cited

Wind-Reprocessed Transients from Stellar-mass Black Hole Tidal Disruption Events

Kyle Kremer, Brenna Mockler, Anthony L. Piro +1

Tidal disruptions of stars by stellar-mass black holes are expected to occur frequently in dense star clusters. Building upon previous studies that performed hydrodynamic simulatio…

astro-ph.SR2023★ 9 cited

Correlating Changes in Spot Filling Factors with Stellar Rotation: The Case of LkCa 4

Facundo Pérez Paolino, Jeffrey S. Bary, Michael S. Petersen +4

We present a multi-epoch spectroscopic study of LkCa 4, a heavily spotted non-accreting T Tauri star. Using SpeX at NASA's Infrared Telescope Facility (IRTF), 12 spectra were colle…

astro-ph.HE2022★ 25 cited

Partial Tidal Disruption of Main-Sequence Stars by Intermediate-Mass Black Holes

Fulya Kıroğlu, James C. Lombardi, Kyle Kremer +3

We study close encounters of a middle-age main-sequence star (modeled using MESA) with massive black holes through hydrodynamic simulations, and explore in particula…

astro-ph.HE2022★ 24 cited

Formation of Low-mass Black Holes and Single Millisecond Pulsars in Globular Clusters

Kyle Kremer, Claire S. Ye, Fulya Kıroğlu +3

Close encounters between neutron stars and main-sequence stars occur in globular clusters and may lead to various outcomes. Here we study encounters resulting in tidal disruption o…

astro-ph.HE2022

Hydrodynamics of Collisions and Close Encounters between Stellar Black Holes and Main-sequence Stars

Kyle Kremer, James C. Lombardi, Wenbin Lu +2

Recent analyses have shown that close encounters between stars and stellar black holes occur frequently in dense star clusters. Depending upon the distance at closest approach, the…

astro-ph.SR2021★ 10 cited

Simulating a stellar contact binary merger -- I. Stellar models

Roger W. M. Hatfull, Natalia Ivanova, James C. Lombardi

We study the initial conditions of a common envelope (CE) event resulting in a stellar merger. A merger's dynamics could be understood through its light curve, but no synthetic lig…