A new model for the continuum spectra of AM CVn binaries and multi-messenger inference with normalizing flows
astro-ph.HE, gr-qc
Submitted: 2026-07-14
Updated: 2026-07-14
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Laser Interferometer Space Antenna
- Astrophysics with the Laser Interferometer Space Antenna
- Prospects for detection of detached double white dwarf binaries with Gaia, LSST and LISA
- LISA verification binaries with updated distances from Gaia Data Release 2
- Galactic binaries with eLISA
- Ultra-compact X-ray Binaries: A Review
- AM CVn stars
- XMM-Newton observations of AM CVn binaries
- V407 Vul: a direct impact accretor
- X-ray luminosity versus orbital period of AM CVn systems
- Galactic Ultracompact X-ray Binaries: Disk Stability and Evolution
- The Advanced X-ray Imaging Satellite
- The Hot and Energetic Universe: A White Paper presenting the science theme motivating the Athena+ mission
- The NewAthena mission concept in the context of the next decade of X-ray astronomy
- LISA Galactic binaries with astrometry from Gaia DR3
- Accreting Double white dwarf binaries: Implications for LISA
- Short-period AM CVn systems as optical, X-ray and gravitational wave sources
- Characterizing accreting double white dwarf binaries with the Laser Interferometer Space Antenna and Gaia
- The gravitational wave signal from the Galactic disk population of binaries containing two compact objects
- The population of AM CVn stars from the Sloan Digital Sky Survey
Related papers
- Numerical Studies of Accretion Flows onto a Neutron Star Engulfed in a Massive Star
- Collisionless Accretion of Finite-Angular-Momentum Plasma onto a Spinning Black Hole
- Impact of Magnetic Field Topology on Electromagnetic and Gravitational Waves from Binary Neutron Star Merger Remnants
- XRISM Resolve Spectroscopy of GX 5-1: Constraints on Iron Spectral Features in a Luminous Neutron-Star Binary
- SN 1006: A Cosmic Laboratory for Investigating Shock Acceleration Physics
- Neutrino Spectral Pinching in 3D Core-Collapse Supernovae: Late-Time Convergence, Failed-Explosion Signatures, and Viewing-Angle Dispersion