Transonic Solutions for Recombination-Driven Stellar Winds

arXiv:2606.21624 · astro-ph.SR · Submitted 2026-06-19 · Read on arXiv

Ilan Strusberg, Re'em Sari, Jim Fuller

astro-ph.SR

Submitted: 2026-06-19

Comments: 12 pages, 5 figures

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

Terminology

• Core — 12× in this paper · explained in 2 episodes
• Accuracy — 3× in this paper · explained in 1 episode
• Common Envelope Interaction — 3× in this paper
• Degeneracy — 1× in this paper · explained in 3 episodes
• Generalization — 1× in this paper · explained in 13 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• Numerical simulations of stellar winds: polytropic models
• Polytropic Gas Effects in Parker's Solar Wind Model and Coronal Hole Flows
• Simulations of common-envelope evolution in binary stellar systems: physical models and numerical techniques
• How negative feedback and the ambient environment limit the influence of recombination in common envelope evolution
• Bridging the gap between luminous red novae and common envelope evolution: the role of recombination energy and radiation force
• The system of ionized gas dynamics
• A global view of post-interaction white dwarf-main sequence binaries
• Steady-state Stellar Winds Driven by Recombination

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?