Influence of mass-transfer stability on the formation of post-common-envelope binaries

arXiv:2606.22927 · astro-ph.SR · Submitted 2026-06-22 · Read on arXiv

Yanxu Shi, Hongwei Ge, Zhenwei Li, Diogo Belloni, Rizhong Zheng, Dengkai Jiang, Hailiang Chen, A. Santos-Garcia, Santiago Torres Gil, Alberto Rebassa-Mansergas, Xuefei Chen, Zhanwen Han

astro-ph.SR

Submitted: 2026-06-22

Comments: Accepted for publication in ApJ

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

Terminology

• Core — 11× in this paper · explained in 2 episodes
• Population Synthesis — 7× in this paper · explained in 2 episodes
• Observational Selection Effects — 6× in this paper · explained in 2 episodes
• Angular Momentum Loss — 3× in this paper · explained in 1 episode
• Chinese Academy of Sciences — 3× in this paper
• Metallicity — 2× in this paper · explained in 3 episodes
• Calibration — 1× in this paper · explained in 7 episodes
• Decoupling — 1× in this paper · explained in 2 episodes
• Sloan Digital Sky Survey — 1× in this paper
• Verification — 1× in this paper · explained in 2 episodes
• alpha — 1× in this paper · explained in 1 episode

Sources

• Mass-Orbital Period Distribution of Massive White Dwarfs Formed Through Stable Mass Transfer

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