V407 Vul: a triple star system with an AM CVn detectable by gravitational wave observatories
James Munday, Antonio C. Rodriguez, Nicole Reindl, Nina Mackensen, Tin Long Sunny Wong, S. P. Littlefair, Ingrid Pelisoli, Alex Brown, N. Castro Segura, Joheen Chakraborty, Harry Dawson, V. S. Dhillon, Matti Dorsch, Martin Dyer, James A. Garbutt, Stephan Geier, Matthew Green, Dan Jarvis, Mark R. Kennedy, Paul Kerry, James McCormac, Steven G. Parsons, Jan van Roestel, Dave Sahman, P. -E. Tremblay, Amalie Yates
astro-ph.SR, astro-ph.HE
Submitted: 2026-07-28
Comments: 16 pages, 7 figures, 5 tables. Resubmitted to A&A after minor revision
License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/
Terminology
Sources
- Science with the Ultraviolet Explorer (UVEX)
- ESO Expanding Horizons White Paper: Electromagnetic characterisation of millihertz gravitational-wave sources in the Milky Way
- The Evolution of Massive Stellar Multiplicity in the Field I. Numerical simulations, long-term evolution and final outcomes
Related papers
- HXI-DLA2: A Physics-Constrained Deep Learning Algorithm for the ASO-S Hard X-ray Imager
- Effect of Neutron Star Jets on Common Envelope Evolution
- Constraining the origin of magnetic white dwarfs
- JW-FD: A 15-Year Multimodal Dataset for Solar Flare Forecasting
- Phlegethon: a fully compressible magnetohydrodynamic code for simulations in stellar astrophysics
- Can MHD Oscillations Modulate Quasi-Periodic Plasma Release from Coronal Streamers?