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20172026
most citedBlack Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties

334 citations · 3k across the 48 of their papers we have counts for

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Showing 2019Show all

7 papers · 1 filter

astro-ph.HE2019★ 300 cited

COSMIC Variance in Binary Population Synthesis

Katelyn Breivik, Scott Coughlin, Michael Zevin +8

The formation and evolution of binary stars is a critical component of several fields in astronomy. The most numerous sources for gravitational wave observatories are inspiraling a…

astro-ph.HE2019★ 214 cited

Modeling Dense Star Clusters in the Milky Way and Beyond with the Cluster Catalog

Kyle Kremer, Claire S. Ye, Nicholas Z. Rui +6

We present a set of 148 independent -body simulations of globular clusters (GCs) computed using the code (). At an age of $\sim10-13…

astro-ph.HE2019★ 151 cited

On the Rate of Neutron Star Binary Mergers from Globular Clusters

Claire S. Ye, Wen-fai Fong, Kyle Kremer +4

The first detection of gravitational waves from a neutron star - neutron star (NS-NS) merger, GW170817, and the increasing number of observations of short gamma-ray bursts (SGRBs)…

astro-ph.HE2019★ 102 cited

The Optical Afterglow of GW170817: An Off-axis Structured Jet and Deep Constraints on a Globular Cluster Origin

Wen-fai Fong, P. K. Blanchard, K. D. Alexander +25

We present a revised and complete optical afterglow light curve of the binary neutron star merger GW170817, enabled by deep Hubble Space Telescope (HST) F606W observations at $\app…

astro-ph.GA2019★ 27 cited

The Role of "Black Hole Burning" in the Evolution of Dense Star Clusters

Kyle Kremer, Claire S. Ye, Sourav Chatterjee +2

As self-gravitating systems, dense star clusters exhibit a natural diffusion of energy from their innermost to outermost regions, which leads to a slow and steady contraction of th…

astro-ph.HE2019★ 334 cited

Black Holes: The Next Generation -- Repeated Mergers in Dense Star Clusters and their Gravitational-Wave Properties

Carl L. Rodriguez, Michael Zevin, Pau Amaro-Seoane +4

When two black holes merge in a dense star cluster, they form a new black hole with a well-defined mass and spin. If that "second-generation" black hole remains in the cluster, it…

astro-ph.HE2019★ 90 cited

Millisecond Pulsars and Black Holes in Globular Clusters

Claire S. Ye, Kyle Kremer, Sourav Chatterjee +2

Over a hundred millisecond radio pulsars (MSPs) have been observed in globular clusters (GCs), motivating theoretical studies of the formation and evolution of these sources throug…