Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters

Single Millisecond Pulsars from Dynamical Interaction Processes in Dense Star Clusters

Globular clusters (GCs) are particularly efficient at forming millisecond pulsars. Among these pulsars, about half lack a companion star, a significantly higher fraction than in the Galactic field. This fraction increases further in some of the densest GCs, especially those that have undergone core...

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Bibliographic Details
Main Authors: Claire S. Ye, Kyle Kremer, Scott M. Ransom, Frederic A. Rasio
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Globular star clusters
Millisecond pulsars
Neutron stars
White dwarf stars
Tidal disruption
N-body simulations
Online Access:https://doi.org/10.3847/1538-4357/ad089a

Internet

https://doi.org/10.3847/1538-4357/ad089a

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