334 citations · 3k across the 48 of their papers we have counts for
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Binary properties of the globular cluster 47 Tuc (NGC 104). A dearth of short-period binaries
Johanna Müller-Horn, Fabian Göttgens, Stefan Dreizler +4
Spectroscopic observations of binary stars in globular clusters are essential to shed light on the poorly constrained period, eccentricity, and mass ratio distributions and to deve…
Predicting the rate of fast radio bursts in globular clusters from binary black hole observations
Aryamann Rao, Claire S. Ye, Maya Fishbach
The repeating fast radio burst (FRB) source in an old globular cluster (GC) in M81 proves that FRBs, which are typically associated with young magnetars, can also occur in old stel…
Can slow pulsars in Milky Way globular clusters form via partial recycling?
Kyle Kremer, Claire S. Ye, Craig O. Heinke +3
Alongside the population of several hundred radio millisecond pulsars currently known in Milky Way globular clusters, a subset of six slowly spinning pulsars (spin periods $0.3-4\,…
Investigating cannibalistic millisecond pulsar binaries using MESA: New constraints from pulsar spin and mass evolution
Devina Misra, Manuel Linares, Claire S. Ye
Compact binary millisecond pulsars (MSPs) with orbital periods d are key to understanding binary evolution involving massive neutron stars (NSs). Due to the ablation of…
Lower-mass-gap Black Holes in Dense Star Clusters
Claire S. Ye, Kyle Kremer, Scott M. Ransom +1
The existence of compact stellar remnants in the mass range has long been debated. This so-called lower mass gap was initially suggested by the lack of low-mass X-…
The Redshift Evolution of the Binary Black Hole Mass Distribution from Dense Star Clusters
Claire S. Ye, Maya Fishbach
Gravitational-wave detectors are unveiling a population of binary black hole (BBH) mergers out to redshifts , and are starting to constrain how the BBH population evol…