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astro-ph.SR2026
The Formation of Very Close Binary Stars
Maxwell Moe
The majority of very close binaries (orbital periods P < 5 days) are in triples. Previous studies surmised that the tertiary hardened the inner binary via Kozai-Lidov cycles couple…
astro-ph.SR2024★ 18 cited
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
Diogo Belloni, Monica Zorotovic, Matthias R. Schreiber +3
In this first in a series of papers related to long-period post-common-envelope (CE) binaries, we investigated whether extra energy is required or not to explain the currently know…
astro-ph.SR2023
Evidence for saturated and disrupted magnetic braking from samples of detached close binaries with M and K dwarfs
Diogo Belloni, Matthias R. Schreiber, Maxwell Moe +2
Context. Recent observations of close detached eclipsing M and K dwarf binaries have provided substantial support for magnetic saturation when stars rotate sufficiently fast, leadi…