Constraining the Galactic Structure Using Time Domain Gravitational Wave Signal from Double White Dwarfs Detected by Space Gravitational Wave Detectors

The gravitational wave (GW) signals from a large number of double white dwarfs (DWDs) in the Galaxy are expected to be detected by space GW detectors, e.g., the Laser Interferometer Space Antenna (LISA), Taiji, and Tianqin in the millihertz band. In this paper, we present an alternative method by di...

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Bibliografische Detailangaben

Hauptverfasser:	Siqi Zhang, Furen Deng, Youjun Lu, Shenghua Yu
Format:	Artigo
Sprache:	Inglês
Veröffentlicht:	IOP Publishing 2024-01-01
Schriftenreihe:	The Astrophysical Journal
Schlagworte:	Gravitational wave sources White dwarf stars Close binary stars Galaxy structure Milky Way Galaxy
Online-Zugang:	https://doi.org/10.3847/1538-4357/ad938a
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