LISA Double White Dwarfs in Triple Systems
astro-ph.SR, astro-ph.HE
Submitted: 2026-09-29
Updated: 2026-09-29
Terminology
Sources
- GW170817: Observation of Gravitational Waves from a Binary Neutron Star Inspiral
- LISA Definition Study Report
- Population synthesis for double white dwarfs I.Close detached systems
- The LISA Gravitational Wave Foreground: A Study of Double White Dwarfs
- Double white dwarfs and LISA
- Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA
- Predicting the LISA white dwarf binary population in the Milky Way with cosmological simulations
- Observationally driven Galactic double white dwarf population for LISA
- Applying the metallicity-dependent binary fraction to double white dwarf formation: Implications for LISA
- Influence of a mass transfer stability criterion on double white dwarf populations
- Predicting gravitational wave signals from BPASS White Dwarf Binary and Black Hole Binary populations of a Milky Way-like galaxy model for LISA
- On the Limb Darkening, Spectral Energy Distribution, and Temperature Structure of Procyon
- The LISA verification binaries
- LISA verification binaries with updated distances from Gaia Data Release 2
- Witscript 2: A System for Generating Improvised Jokes Without Wordplay
- Short-period AM CVn systems as optical, X-ray and gravitational wave sources
- Supernova Type Ia progenitors from merging double white dwarfs: Using a new population synthesis model
- The Evolution of Compact Binary Star Systems
- The evolution of stellar triples: The most common evolutionary pathways
- A Test of Spectroscopic Age Estimates of White Dwarfs using Wide WD+WD Binaries
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