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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發表在:	The Astrophysical Journal
Main Authors:	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
格式:	Article
語言:	英语
出版:	IOP Publishing 2024-01-01
主題:	White dwarf stars Compact binary stars Semi-detached binary stars Gravitational wave sources
在線閱讀:	https://doi.org/10.3847/1538-4357/ad2068