Positive superhumps in high mass ratio cataclysmic variables driven by apsidal disk precession

arXiv:2607.14307 · astro-ph.SR · Submitted 2026-07-15 · Read on arXiv

Rebecca G. Martin, Stephen H. Lubow, David Vallet, Stephen Lepp

astro-ph.SR

Submitted: 2026-07-15

Comments: Accepted for publication in ApJL

License: http://arxiv.org/licenses/nonexclusive-distrib/1.0/

Terminology

• Bulk Viscosity — 1× in this paper · explained in 2 episodes
• Cataclysmic Variables (CVs) — 1× in this paper · explained in 2 episodes

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?