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Formation of Long-Period Post-Common-envelope Binaries I. No Extra Energy is Needed to Explain Oxygen-Neon White Dwarfs Paired with AFGK-type Main-Sequence Stars

ASTRONOMY & ASTROPHYSICS(2024)

Cited 9|Views25
Key words
methods: numerical,stars: AGB and post-AGB,binaries: general,stars: evolution,white dwarfs
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