The Common Envelope Evolution Outcome. III. the Improvement of Stellar Binding Energy with the Envelope Residual

arXiv:2609.24010 · astro-ph.SR · Submitted 2026-09-21 · Read on arXiv

astro-ph.SR

Submitted: 2026-09-21

Updated: 2026-09-21

Comments: 15 pages, 9 figures

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

Terminology

• Core — 60× in this paper · explained in 2 episodes
• Accuracy — 7× in this paper · explained in 1 episode
• Population Synthesis — 5× in this paper · explained in 2 episodes
• Metallicity — 4× in this paper · explained in 3 episodes
• Abundance — 1× in this paper · explained in 1 episode
• Trace — 1× in this paper · explained in 2 episodes

Sources

• Unveiling the properties of pulsating low-mass helium-core white dwarfs through TESS asteroseismology I. First results
• Stability Criteria for Mass Transfer in Binary Stellar Evolution
• Physics of Binary Star Evolution -- from Stars to X-ray Binaries and Gravitational Wave Sources

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