Beyond the Background: Gravitational-wave Anisotropy and Continuous Waves from Supermassive Black Hole Binaries

Beyond the Background: Gravitational-wave Anisotropy and Continuous Waves from Supermassive Black Hole Binaries

Pulsar timing arrays have found evidence for a low-frequency gravitational-wave background (GWB). Assuming that the GWB is produced by supermassive black hole binaries (SMBHBs), the next gravitational-wave (GW) signals astronomers anticipate are continuous waves (CWs) from single SMBHBs and their as...

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Bibliographic Details
Main Authors: Emiko C. Gardiner, Luke Zoltan Kelley, Anna-Malin Lemke, Andrea Mitridate
Format: Article
Language:English
Published: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Subjects:
Gravitational waves
Supermassive black holes
Galaxies
Online Access:https://doi.org/10.3847/1538-4357/ad2be8

Internet

https://doi.org/10.3847/1538-4357/ad2be8

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