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LISA Galactic Binaries with Astrometry from Gaia DR3

Galactic compact binaries with orbital periods shorter than a few hours emit detectable gravitational waves (GWs) at low frequencies. Their GW signals can be detected with the future Laser Interferometer Space Antenna (LISA). Crucially, they may be useful in the early months of the mission operation...

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Gardado en:
Principais autores: Thomas Kupfer, Valeriya Korol, Tyson B. Littenberg, Sweta Shah, Etienne Savalle, Paul J. Groot, Thomas R. Marsh, Maude Le Jeune, Gijs Nelemans, Anna F. Pala, Antoine Petiteau, Gavin Ramsay, Danny Steeghs, Stanislav Babak
Formato: Artigo
Idioma:Inglês
Publicado: IOP Publishing 2024-01-01
Series:The Astrophysical Journal
Assuntos:
White dwarf stars
Compact binary stars
Semi-detached binary stars
Gravitational wave sources
Acceso en liña:https://doi.org/10.3847/1538-4357/ad2068
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