A Multimessenger Mass Determination Method for LISA Neutron Star–White Dwarf Binaries

A Multimessenger Mass Determination Method for LISA Neutron Star–White Dwarf Binaries

Determining the masses of neutron stars (NSs) accurately improves our understanding of the NS interior and complicated binary evolution. However, the masses of the systems are degenerate with the orbital inclination angle when using solely gravitational waves (GWs) or electromagnetic measurements, e...

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Bibliographic Details
Main Authors: Kaye Jiale Li, Jane SiNan Long, Kinwah Wu, Albert K. H. Kong
Format: Article
Language:English
Published: IOP Publishing 2025-01-01
Series:The Astrophysical Journal
Subjects:
Neutron stars
Compact binary stars
Gravitational waves
Online Access:https://doi.org/10.3847/1538-4357/adc0fd
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