activity
20182021
most citedOn the Rate of Neutron Star Binary Mergers from Globular Clusters

151 citations · 574 across the 8 of their papers we have counts for

collaborators

21 papers

astro-ph.GA202157 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

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.HE202142 cited

The Observed Rate of Binary Black Hole Mergers can be Entirely Explained by Globular Clusters

Carl L. Rodriguez, Kyle Kremer, Sourav Chatterjee +5

Since the first signal in 2015, the gravitational-wave detections of merging binary black holes (BBHs) by the LIGO and Virgo collaborations (LVC) have completely transformed our un…

astro-ph.HE2021102 cited

Intermediate-mass Black Holes from High Massive-star Binary Fractions in Young Star Clusters

Elena González, Kyle Kremer, Sourav Chatterjee +5

Black holes formed in dense star clusters, where dynamical interactions are frequent, may have fundamentally different properties than those formed through isolated stellar evoluti…

astro-ph.GA202146 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…

astro-ph.HE2020

Fast Optical Transients from Stellar-Mass Black Hole Tidal Disruption Events in Young Star Clusters

Kyle Kremer, Wenbin Lu, Anthony L. Piro +3

Observational evidence suggests that the majority of stars may have been born in stellar clusters or associations. Within these dense environments, dynamical interactions lead to h…